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Type of variable star
slow irregular variable (ascribed the GCVS types L, LB and LC) is a variable star that exhibit no or very poorly defined periodicity in their slowly changing
Slow_irregular_variable
Type of variable star
these come in subgroups ISA and ISB. Pulsating irregular giants or supergiants, called slow irregular variables, are all of late spectral types (K, M, C, or
Irregular_variable
Type of variable star
slow irregular variable by the GCVS, but reported to be of SRb type by later research. These four are all class M giants, although some SRb variables
Semiregular_variable_star
Star in the constellation Cepheus
solar radii, making it one of the largest known stars. It is a slow irregular variable with an apparent magnitude that ranges between 10.55 - 11.4. "All-Sky
V355_Cephei
Star whose brightness fluctuates, as seen from Earth
variables are very closely related to Mira variables, possibly the only difference being pulsating in a different harmonic. Slow irregular variables These
Variable_star
Cool luminous pulsating variable star
period variables. At its broadest, LPVs include Mira, semiregular, slow irregular variables, and OGLE small amplitude red giants (OSARGs), including both giant
Long-period_variable_star
Binary star in the constellation Dorado
variability has since been observed to transition from semi-regular to irregular circa 2014. WOH G64 A was discovered to be a prominent source of OH, H
WOH_G64
Star in the constellation Crux
DU Crucis is a red supergiant and slow irregular variable star in the open cluster NGC 4755, which is also known as the Kappa (κ) Crucis Cluster or Jewel
DU_Crucis
"General Catalog of Variable Stars (GCVS database, version 2012Apr)". Retrieved 2013-03-30. "AAVSO Website". American Association of Variable Star Observers
List_of_stars_in_Columba
Star in the constellation Canis Major
classed as a type LC slow irregular variable star in the American Association of Variable Star Observers (AAVSO) Variable Star Index. Other periods of
VY_Canis_Majoris
Binary star in the constellation Scorpius
Distinctly reddish when viewed with the naked eye, Antares is a slow irregular variable star that ranges in brightness from an apparent visual magnitude
Antares
Slow irregular variable; Corona Australis
one lasting 5.37 days and the other lasting 71.1 days. It is a slow irregular variable of subtype Lb that fluctuates between 5.45 and 5.51 in the Hipparcos
V718_Coronae_Australis
Star in the constellation Puppis
it the orange hue of a K-type star. It shows the behavior of a slow irregular variable. In addition to its binary components, Sigma Puppis has a more
Sigma_Puppis
Taurus Brightest Star
030 mas. Aldebaran is a slightly variable star, assigned to the slow irregular type LB. The General Catalogue of Variable Stars indicates variation between
Aldebaran
Star in the constellation Andromeda
identified as a long-period variable in 1999 from analysis of Hipparcos photometry. It was classified as a slow irregular variable, but analysis of its light
V385_Andromedae
Constellation in the southern celestial hemisphere
a yellow hypergiant, one of the rarest types of stars. It is a slow irregular variable, with a minimum magnitude of 4.05 and a maximum magnitude of 3
Carina_(constellation)
Star in the constellation Cygnus
degree south of another variable red supergiant, BC Cygni. BI Cyg is a slow irregular variable star classified as type Lc, an irregular supergiant. Its brightness
BI_Cygni
Single variable star in the constellation Camelopardalis
of M4IIIa. Its variable nature was discovered by American astronomer J. Ashbrook in 1948. This is a suspected slow irregular variable of sub-type Lb that
VZ_Camelopardalis
Binary star in the constellation Phoenix
Phoenicis is listed in the General Catalogue of Variable Stars as a possible slow irregular variable with a range from 3.39 to 3.49, the same as reported
Gamma_Phoenicis
Star in the constellation Lacerta
as slow variations with a period of 1,100 or 1,601 days. Although listed in the General Catalogue of Variable Stars as a slow irregular variable, it
V424_Lacertae
Star in constellation Canes Venatici
giant star with a stellar classification of M3- IIIa. It is a slow irregular variable of type Lb, with a brightness that ranges between magnitudes 4
AW_Canum_Venaticorum
Catalogue of Variable Stars (GCVS4.2)". Retrieved 10 April 2012. Samus, N. N.; Durlevich, O. V.; et al. (2012). "General Catalog of Variable Stars (GCVS
List_of_stars_in_Cassiopeia
Star in the constellation Octans
listed in the General Catalogue of Variable Stars as a possible slow irregular variable. It was classified as a variable star in 1977, on the basis of a
BQ_Octantis
Star in the constellation Vulpecula
typical orange color of a K-type star. NR Vulpeculae is also a slow irregular variable, with an apparent magnitude ranging from 9.13 to 9.61. It is considered
NR_Vulpeculae
Red giant star in the constellation Lynx
sequence. It has been classified as a possible slow irregular variable, after being found to be slightly variable in 1969 by Olin J. Eggen. Its changes in brightness
1_Lyncis
Star in the northern constellation of Pegasus
it the orange-hued glow of a K-type star. Epsilon Pegasi is a slow irregular variable star that usually has a brightness between magnitudes 2.37 and
Epsilon_Pegasi
Star in the constellation Tucana
present it has 49 times the Sun's radius. It is classified as a slow irregular variable and its brightness varies from magnitude +4.75 to +4.93. Cyclical
Nu_Tucanae
Star in the constellation Lacerta
constellation Lacerta. Its apparent magnitude is 4.36. 5 Lacertae is a slow irregular variable star with a small amplitude. Photometry from the Hipparcos satellite
5_Lacertae
Star in the constellation of Sagittarius
star as a variable star in his Uranometria Argentina. It was given its variable star designation in 1973. It is a slow irregular variable with multiple
62_Sagittarii
Variable star in the constellation Canis Major
confirmed in 1963, and it was formally catalogued as a variable star. It is classified as an irregular variable star and its brightness varies from magnitude +3
Sigma_Canis_Majoris
Star in the constellation Cetus
7 Ceti. It was given its variable star designation in 1973. Samus et al. (2017) has it classed as a slow irregular variable of type LB:, and ranges in
7_Ceti
Carbon star visible to the naked eye in the constellation Pisces
Piscium varies between +4.9 and +5.5 and it is classified as a slow irregular variable. Photometry has shown some periodicity in the brightness of 224
TX_Piscium
Archived from the original on 2012-02-27. Retrieved 2010-07-16. "AAVSO Website". American Association of Variable Star Observers. Retrieved 9 March 2014.
List_of_stars_in_Monoceros
Star in the constellation Canis Major
−11° 1805, is a variable star. It was given its variable star designation, W Canis Majoris, in 1912. W CMa is classified as a slow irregular variable star. Detailed
W_Canis_Majoris
Star in the Small Magellanic Cloud in the constellation Tucana
the infrared. It is listed in the General Catalogue of Variable Stars as a slow irregular variable, but a period of 720 days has been calculated, as well
HV_11423
Triple star in the constellation Puppis
photosphere at an effective temperature of 3,660 K. It shows small amplitude irregular pulsations, and also some variation associated with the orbital motion
KQ_Puppis
Star in the constellation Norma
39 ly). HD 143183 is catalogued with the variable star designation V558 Normae as its brightness varies irregularly between apparent magnitudes 7.3 and 8
HD_143183
Variable star in the constellation Cygnus
velocity of −24 km/s. The primary, component A, is a variable star, most likely of the slow irregular type, which ranges in magnitude from 4.91 down to 4
T_Cygni
Star in the constellation Centaurus
classification of M3/4III. Samus et al. (2017) classify this as a slow irregular variable of sub-type Lb and its brightness varies from magnitude +5.52 down
V763_Centauri
Star in the constellation Andromeda
literature about what class of variable star EU Andromedae belongs to, with some researchers listing it as a slow irregular variable, and others listing it as
EU_Andromedae
Star in the constellation Cepheus
Cephei is a red supergiant star located within the Milky Way. It is an irregular variable located over 13,000 light-years away from the Sun. It has an estimated
V354_Cephei
Star in the constellation Carina
BO Carinae, also known as HD 93420, is an irregular variable star in the constellation Carina. BO Car has a maximum apparent magnitude of +7.18. Its distance
BO_Carinae
Star in the constellation Gemini
magnitudes by extinction from intervening gas and dust. It is a slow irregular variable of type LB. Its brightness varies between magnitude +2.75 and +3
Mu_Geminorum
Catalogue of Variable Stars (GCVS4.2)". Retrieved 2 April 2012. Samus, N. N.; Durlevich, O. V.; et al. (2012). "General Catalog of Variable Stars (GCVS
List_of_stars_in_Ara
Binary star system in the constellation Eridanus
giant branch with a stellar classification of M3/4 III. It is a slow irregular variable star of type Lb, undergoing changes in magnitude over the range
Tau4_Eridani
52497 33927 07h 02m 24.78s +24° 12′ 55.6″ 5.20 −3.33 1655 G5II slow irregular variable, Vmax = 5.18m, Vmin = 5.20m 63 Gem 63 58728 36238 07h 27m 44.39s
List_of_stars_in_Gemini
Star in the constellation Volans
820 K, which gives it a red glow. HD 77887 is suspected to be a slow irregular variable whose brightness fluctuates at a tenth of a magnitude. Koen and
HD_77887
Star in the constellation Camelopardalis
giving a red hue. CQ Cam has been classified as a low amplitude slow irregular variable based on Hipparcos photometry. However, there have not been enough
CQ_Camelopardalis
Star in the constellation Carina
Cygni variable. A period of 556 days was suggested, but it is not entirely consistent. It is now generally treated as a semiregular or irregular supergiant
V382_Carinae
Evolved K-type star in the constellation of Vela
giving it the cool orange hue of a K-type star. It is an Lc-type, slow irregular variable star with its brightness varying between apparent magnitudes +2
Lambda_Velorum
Constellation in the southern celestial hemisphere
apparent magnitude 4.71 and 4.76, and has been classified as a slow, irregular variable. Near Mu is Lambda Muscae, the third-brightest star in the constellation
Musca
Catalogue of Variable Stars (GCVS4.2)". Retrieved 3 April 2012. Samus, N. N.; Durlevich, O. V.; et al. (2012). "General Catalog of Variable Stars (GCVS
List of stars in Camelopardalis
List_of_stars_in_Camelopardalis
Star in the constellation Aquarius
effective strength measured at 220±60 Gauss. It is classified as slow irregular variable and pulsation periods of 24.5, 32.0, and 49.5 days have been identified
Lambda_Aquarii
Star in the constellation Camelopardalis
star, then called HR 1105, is a variable star, based on observations made at Washburn Observatory. It was given its variable star designation, BD Camelopardalis
BD_Camelopardalis
Star in the constellation Boötes
parallax measurements, it is about 540 light-years distant. This is a slow irregular variable with an apparent magnitude varying between 4.98 and 5.33. The variability
HD_123657
Star in the constellation Vela
The star was found to be a variable star when the Hipparcos data was analyzed, in 1996. It is a slow irregular variable of type LC with a frequency of
GZ_Velorum
Star in the constellation Sagittarius
the helium at its core. This star is classified as an oxygen-rich irregular variable, as it undergoes small magnitude fluctuations between +3.08 and 3
Eta_Sagittarii
Star in the constellation Andromeda
carbon star in the constellation of Andromeda. It is a variable star classified as a slow irregular pulsating supergiant, and varies from an apparent visual
SU_Andromedae
Variable star in the constellation Canis Major
is an orange K-type supergiant of spectral type K2.5 Iab and is an irregular variable star, varying between apparent magnitudes 3.78 and 3.99. A cool star
Omicron1_Canis_Majoris
Star in the constellation Carina
a variable star when the Hipparcos data was analyzed, and for that reason it was given a variable star designation in 1999. It is a slow irregular variable
V520_Carinae
Variable star in the constellation Eridanus
abbreviated Gamma Eri, γ Eri), formally named Zaurak /ˈzɔːræk/, is a variable star in the constellation of Eridanus. It is visible to the naked eye with
Gamma_Eridani
Star in the constellation Carina
given its variable star designation in 1999. It is classified as a slow irregular variable whose prototype is TZ Cassiopeiae. List of largest known stars
V528_Carinae
Star in the constellation Auriga
approximately 219 times the size of the Sun. It is classified as a slow irregular variable of type LC and its brightness varies from magnitude +4.24 to +4
Pi_Aurigae
Red giant star in the constellation Cancer
discovery that Mu1 Cancri is a variable star. It was given its variable star designation in 1972. It is a slow irregular variable with thermal pulsation periods
Mu1_Cancri
Star in the constellation Cassiopeia
Cassiopeiae was reported as being variable by Williamina Fleming and published posthumously in 1911. It is a slow irregular variable star with a possible period
TZ_Cassiopeiae
Star in the constellation Cygnus
detected from this system in 1985/86. The supergiant primary is a slow irregular variable with an amplitude of about 0.1 magnitudes. Its angular diameter
47_Cygni
Comparison of a wide range of volumes
3×1035 Estimated volume of S Orionis 1.5×1035 Volume of Antares, a slow irregular variable in Scorpius ~2.75×1035 Volume of Betelgeuse 1×1036 One cubic terametre
Orders_of_magnitude_(volume)
Catalogue of Variable Stars (GCVS4.2)". Retrieved 8 April 2012. Samus, N. N.; Durlevich, O. V.; et al. (2012). "General Catalog of Variable Stars (GCVS
List_of_stars_in_Capricornus
Star in the constellation Cygnus
KY Cygni is a variable red supergiant or hypergiant of spectral class M3Ia located in the constellation Cygnus. It is approximately 4,700 light-years away
KY_Cygni
Overview of the scientific field of astronomy
Cephei variable PV Telescopii variable Long Period and Semiregular Mira variable Semiregular variable Slow irregular variable Other RV Tauri variable Alpha
Outline_of_astronomy
Red Supergiant star in the constellation Perseus
constellation of Perseus in the northern celestial hemisphere. Classified as a variable star of spectral type M1-Iab-Ib, it exhibits mild brightness variations
PR_Persei
Star in the constellation Cassiopeia
year to year and the star has been classified as irregular. The optical variability is dominated by slow pulsation with 83.8 d period, overlapped by faster
IRAS_23304+6147
Triple star system in the constellation Scutum
but is now though to be a detached eclipsing binary with additional irregular pulsations of the cool supergiant. Another star system similar to FR Scuti
FR_Scuti
Star in the constellation Boötes
cooled and expanded off the main sequence. It is classified as a slow irregular variable of the Lb type, and its brightness has been observed to vary from
13_Boötis
2012-02-27. Retrieved 2010-07-16. "AAVSO Website". American Association of Variable Star Observers. Retrieved 9 March 2014. "Naming Stars". Retrieved 13 December
List_of_stars_in_Scorpius
Star in the constellation Carina
Jump Cannon's 1907 work, Second Catalogue of Variable Stars. It is catalogued as an irregular variable star, but a number of possible pulsation periods
RT_Carinae
42973 29919 06h 17m 54.83s +61° 30′ 55.1″ 4.95 −1.34 590 M3III slow irregular variable, ΔV = 0.11m HD 56169 56169 35384 07h 18m 31.98s +49° 27′ 53.1″
List_of_stars_in_Lynx
Star in the constellation of Cepheus
the star is a variable star. That same year it was given its variable star designation, ST Cephei. Listed as an LC irregular variable star, the brightness
ST_Cephei
Star in the constellation Auriga
Aurigae is listed in the General Catalogue of Variable Stars as a slow irregular variable, indicating that no regularity could be found in the brightness variations
NO_Aurigae
Star in the constellation Carina
discovery that the star's brightness varies, in 1970. It was given its variable star designation, V341 Carinae, in 1975. HD 65750 is located about 900
HD_65750
Star in the constellation of Columba
designation, AF Columbae, in 1999. The object is classified as a slow irregular variable of subtype Lb. Tabur et al. (2009) found 5 periods for AF Columbae
AF_Columbae
Star in the constellation Draco
giant star with a stellar classification of M3.5 III. It is a periodic variable with a frequency of 11.98912 cycles per day and an amplitude of 0.0254
10_Draconis
Star in the constellation Aquarius
LP Aquarii is a pulsating variable star in the constellation of Aquarius that varies between magnitudes 6.30 and 6.64. The position of the star near the
LP_Aquarii
Variable star in the constellation Virgo
giant star with a stellar classification of M3 IIICa-1. It is an irregular variable with seven measured pulsation periods ranging from 22.4 to 162.6 days
Psi_Virginis
Star in the constellation Boötes
to around 210 times the Sun's radius. EK Boo is classified as a slow irregular variable that ranges in luminosity with an amplitude of 0.38 in magnitude
HD_130144
Red supergiant star in the constellation of Puppis
V.; et al. (2009). "VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)". VizieR On-line Data Catalog: B/GCVS. Originally
MZ_Puppis
Type of cool giant star
star. It is a slow irregular variable in a symbiotic binary system with a hotter companion which may also be variable. The Mira variable Chi Cygni is an
S-type_star
de Données astronomiques de Strasbourg. Retrieved 2007-01-03. "AAVSO Website". American Association of Variable Star Observers. Retrieved 9 March 2014.
List_of_stars_in_Lacerta
Red giant star in the constellation Eridanus
M1 III, and is currently on the asymptotic giant branch. It is a slow irregular variable type LB that can increase in magnitude up to 4.38. The measured
Pi_Eridani
Binary star in the constellation Carina
Apparent magnitude (H) 3.432±0.208 Apparent magnitude (K) 2.970±0.236 Variable type LC Primary Evolutionary stage Post-red supergiant Spectral type A7Ie–F0:I
AFGL_4106
N. N.; Durlevich, O. V.; et al. (2004). "Combined General Catalogue of Variable Stars (GCVS4.2)". Retrieved 2007-01-03. Gould, B. A. "Uranometria Argentina"
List_of_stars_in_Crux
Triple star system in the constellation Cepheus
slightly variable between 5.5 and 5.7. It is faintly visible to the naked eye under good observing conditions. The star was discovered to be a variable star
V381_Cephei
Star in the constellation Pisces
30 Piscium (HIP 154) is a solitary variable star in the zodiac constellation of Pisces. It is visible to the naked eye with an apparent visual magnitude
30_Piscium
Archived from the original on 2012-02-27. Retrieved 2010-07-16. "AAVSO Website". American Association of Variable Star Observers. Retrieved 9 March 2014.
List_of_stars_in_Telescopium
Star in the constellation Draco
a stellar classification of M0III-IIIa Ca1. It is a suspected slow irregular variable with a periodicity of roughly 1,100 days. It has an estimated 1
Lambda_Draconis
Svolopoulos, Sotirios (1988). "Spectral types of 80 early-type stars of variable radial velocity". Astronomical Society of the Pacific. 100: 828. Bibcode:1988PASP
List_of_stars_in_Cancer
Portion of the giant branch before helium ignition
magnitudes, semiregular variables with less obvious periods or multiple periods and slightly lower amplitudes, and slow irregular variables with no obvious period
Red-giant_branch
Star in the constellation Auriga
supergiant star with a stellar classification of K5-M1Iab-Ib. It is a slow irregular variable of the LC type, with its brightness varying in magnitude by 0.44
Psi1_Aurigae
Star in the constellation Cygnus
Sun. When V1027 Cygni was first noticed as a variable star, it was thought to be an irregular variable, dimming and brightening erratically with no discernible
V1027_Cygni
Catalogue of Variable Stars (GCVS4.2)". Retrieved 30 July 2012. Samus, N. N.; Durlevich, O. V.; et al. (2012). "General Catalog of Variable Stars (GCVS
List_of_stars_in_Triangulum
SLOW IRREGULAR-VARIABLE
SLOW IRREGULAR-VARIABLE
Surname or Lastname
English
English : from Middle English blowe, blaa, bloo ‘pale’, hence a nickname for someone with an exceptionally pale complexion.Americanized spelling of French Bleau.
Boy/Male
African, Hindu, Indian, Punjabi, Sanskrit, Sikh, Swahili
Slow; Firm
Girl/Female
Indian
Grateful
Girl/Female
Indian, Telugu
Slow and Steady
Girl/Female
Welsh
Slow.
Boy/Male
Hindu, Indian, Tamil
Regular Winner
Surname or Lastname
English
English : nickname denoting someone with very white hair or an exceptionally pale complexion, from Old English snÄw ‘snow’.Americanized and shortened form of any of the Jewish ornamental names composed with German Schnee, Schnei, Schneu ‘snow’ as the first element.
Surname or Lastname
English
English : variant of Clough.English : metonymic occupational name for a nailer, from Old French clou ‘nail’. Compare Clower.Possibly an Americanized spelling of German Klau, a habitational name for someone from Klau near Aachen or Clauen in Lower Saxony, or Glau, a nickname for an astute person, from Old High German, Low German glou, glau ‘circumspect’.
Boy/Male
Hindu, Indian
Slow
Surname or Lastname
English (Lancashire)
English (Lancashire) : unexplained.Perhaps an Americanized spelling of Schau.
Boy/Male
Indian, Sanskrit
Not Slow; Agile; Rapid
Boy/Male
Indian, Sanskrit
Making Slow Progress
Boy/Male
Indian
Chant; Mantra
Surname or Lastname
English
English : unexplained; possibly a variant of Flew, a metonymic occupational name for a fisherman, from Middle English flue, denoting a kind of fishing net.
Girl/Female
American, Australian, Chinese, Latin, Spanish
Snowy; Covered with Snow; Snow-covered; Snowfall; Snow-capped; Snow-clad; Snow Capped
Boy/Male
British, English
Laurel
Surname or Lastname
English (Devon)
English (Devon) : unexplained. Possibly an irregular variant of Birchall.
Surname or Lastname
English and Scottish
English and Scottish : topographic name for someone who lived near a tumulus, mound or hill, Middle English lowe, from Old English hlÄw (see Law 2).Scottish and English : nickname for a short man, from Middle English lah, lowe (Old Norse lágr; the word was adopted first into the northern dialects of Middle English, where Scandinavian influence was strong, and then spread south, with regular alteration of the vowel quality).English and Scottish (of Norman origin) : nickname for a violent or dangerous person, from Anglo-Norman French lou, leu ‘wolf’ (Latin lupus). Wolves were relatively common in Britain at the time when most surnames were formed, as there still existed large tracts of uncleared forest.Scottish : from a pet form of Lawrence. Compare Lowry 1.Americanized spelling of Jewish Lowe.
Surname or Lastname
English
English : variant of Stowe.
Boy/Male
Shakespearean
King Henry IV, Part 1 and 2' An irregular humorist.
SLOW IRREGULAR-VARIABLE
SLOW IRREGULAR-VARIABLE
Girl/Female
Hindu, Indian, Marathi
Pearl; The Moon
Boy/Male
British, English, Italian
Dark of Skin
Boy/Male
Muslim/Islamic
Fearless
Girl/Female
Tamil
Lord of Kashi, Another name for Shiva, Attraction
Girl/Female
Muslim/Islamic
Imaginary picture
Male
Scandinavian
Scandinavian form of Old Norse Hallvar�r, HALVARD means "rock defender."
Surname or Lastname
German
German : metonymic occupational name for the owner of a tavern or a nickname for a drinker, from Low German tappe ‘tap’.German : variant of Tapp.English : variant spelling of Tapp.
Boy/Male
Native American
Blackbird.
Boy/Male
Scottish American
From Hugh's town. Place-name and surname. American West Texan general Sam Houston. A city in...
Girl/Female
Hindu, Indian, Kannada, Marathi, Sanskrit, Sindhi, Tamil, Telugu
Of Intelligence
SLOW IRREGULAR-VARIABLE
SLOW IRREGULAR-VARIABLE
SLOW IRREGULAR-VARIABLE
SLOW IRREGULAR-VARIABLE
SLOW IRREGULAR-VARIABLE
a.
Irregular in position; having no regular order; as, scattered leaves.
v. t.
To scatter like snow; to cover with, or as with, snow.
a.
Thorough; complete; unmitigated; as, a regular humbug.
superl.
Moving a short space in a relatively long time; not swift; not quick in motion; not rapid; moderate; deliberate; as, a slow stream; a slow motion.
n.
A low-lying piece of watery land; -- called also flow moss and flow bog.
v. t.
To render slow; to slacken the speed of; to retard; to delay; as, to slow a steamer.
a.
Not regular; not conforming to a law, method, or usage recognized as the general rule; not according to common form; not conformable to nature, to the rules of moral rectitude, or to established principles; not normal; unnatural; immethodical; unsymmetrical; erratic; no straight; not uniform; as, an irregular line; an irregular figure; an irregular verse; an irregular physician; an irregular proceeding; irregular motion; irregular conduct, etc. Cf. Regular.
a.
Having all the parts of the same kind alike in size and shape; as, a regular flower; a regular sea urchin.
v. t.
To make irregular; to disorder.
superl.
Behind in time; indicating a time earlier than the true time; as, the clock or watch is slow.
adv.
In an irregular manner.
v. t.
To form by inflation; to swell by injecting air; as, to blow bubbles; to blow glass.
v. t.
To transport in a scow.
a.
Constituted, selected, or conducted in conformity with established usages, rules, or discipline; duly authorized; permanently organized; as, a regular meeting; a regular physican; a regular nomination; regular troops.
superl.
Not ready; not prompt or quick; dilatory; sluggish; as, slow of speech, and slow of tongue.
a.
Conformed to a rule; agreeable to an established rule, law, principle, or type, or to established customary forms; normal; symmetrical; as, a regular verse in poetry; a regular piece of music; a regular verb; regular practice of law or medicine; a regular building.
n.
One who is not regular; especially, a soldier not in regular service.
superl.
Not advancing or improving rapidly; as, the slow growth of arts and sciences.
v. t.
To put out of breath; to cause to blow from fatigue; as, to blow a horse.