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Star system in the constellation Cassiopeia
Gamma Cassiopeiae, Latinized from γ Cassiopeiae formally named Tiansi, is a multiple star system at the center of the distinctive "W" asterism in the
Gamma_Cassiopeiae
Type of eruptive variable star
A Gamma Cassiopeiae variable (γ Cassiopeiae variable) is a type of variable star, named for its prototype γ Cassiopeiae. The General Catalogue of Variable
Gamma_Cassiopeiae_variable
Type of star
disappearance of, the "shell" are called Gamma Cassiopeiae variables. Pleione and Gamma Cassiopeiae itself are both variable stars that have intermittent shell
Shell_star
Constellation in the northern celestial hemisphere
Beta, and Gamma Cassiopeiae were named. Alpha Cassiopeiae was called Poloahilani, Beta Cassiopeiae was called Polula, and Gamma Cassiopeiae was called
Cassiopeia_(constellation)
Second-brightest star in the constellation Cassiopeia
Beta Cassiopeiae is a Delta Scuti variable star in the constellation of Cassiopeia. It has the proper name Caph, pronounced /ˈkæf/; Beta Cassiopeiae is
Beta_Cassiopeiae
Star whose brightness fluctuates, as seen from Earth
appear to be stochastic while others show multiple periods. Gamma Cassiopeiae (γ Cas) variables are non-supergiant fast-rotating B class emission line-type
Variable_star
Binary star in the Pleiades star cluster
small amount (~1/6 magnitude). Pleione is now classified as a Gamma Cassiopeiae type variable star, with brightness fluctuations that range between a 4.8
Pleione_(star)
Binary star system in the constellation Scorpius
space anywhere in the main ring system." Delta Scorpii A is a Gamma Cassiopeiae variable star. This type of star shows irregular slow brightness variations
Delta_Scorpii
Star in the constellation Cassiopeia
binary is a blue-white B-type giant star. It is classified as a Gamma Cassiopeiae variable and its brightness varies from magnitude 4.30 to 4.62. It is rotating
Omicron_Cassiopeiae
O-type main sequence star in the constellation Ophiuchus
luminosity is varying in a periodic manner similar to that of a Beta Cephei variable. This periodicity has a dozen or more frequencies ranging between 1–10
Zeta_Ophiuchi
Zodiac constellation straddling the celestial equator
Psc), 349 lightyears, class G7 IIIa, magnitude 3.62. It is a Gamma Cassiopeiae variable with a weak magnetic field. Torcular ("thread"), otherwise Omicron
Pisces_(constellation)
Star in the constellation Centaurus
slightly variable, and it is classified as a Gamma Cassiopeiae variable star with multiple periods of variability. The International Variable Star Index
Eta_Centauri
Star in the constellation Cassiopeia
Epsilon Cassiopeiae is a single star in the northern constellation of Cassiopeia. It has the proper name Segin, pronounced /ˈsɛɡɪn/; Epsilon Cassiopeiae is
Epsilon_Cassiopeiae
Star in the constellation Canis Minor
variability, and in 1977 it was classified as a γ Cassiopeiae variable in the General Catalogue of Variable Stars. A number of studies have found no variation
Beta_Canis_Minoris
Star in the constellation Ara
BE, indicating that it is a variable Be star but not obviously a Gamma Cassiopeiae variable. The International Variable Star Index defines it as GCAS
Alpha_Arae
B-type star with emission lines
visually and spectroscopically variable. Be stars can be classified as Gamma Cassiopeiae variables when a transient or variable disk is observed. Be stars
Be_star
Variable star in the constellation Canis Major
to the naked eye of an observer far from city lights. It is a Gamma Cassiopeiae variable star, whose brightness varies from magnitude 4.8 to 6.25. In 1967
FY_Canis_Majoris
Star in the constellation Cygnus
ṣadr "chest", the same word which gave rise to the star Schedar (Alpha Cassiopeiae). In 2016, the International Astronomical Union organized a Working Group
Gamma_Cygni
Star system in the constellation Vela
absorption lines) it is also dubbed the Spectral Gem of Southern Skies. Gamma Cassiopeiae, informally named Navi for astronaut Virgil Ivan "Gus" Grissom Iota
Gamma_Velorum
Binary star in the constellation Taurus
brightness. The General Catalogue of Variable Stars lists it as an eclipsing variable and a Gamma Cassiopeiae variable, but it may not be either. Hrvoje
Zeta_Tauri
Constellation in the southern celestial hemisphere
each other as viewed from Earth, they are unrelated. Kappa is a Gamma Cassiopeiae variable of spectral type B2Vne, which brightened by 50% between 1963 and
Canis_Major
Star in the constellation Puppis
classified as a Gamma Cassiopeiae variable. It is approximately 930 light years away based on parallax. MX Puppis was first found to be a variable star by Alan
MX_Puppis
Constellation in the northern celestial hemisphere
variations are slight, Gomeisa is classified as a shell star (Gamma Cassiopeiae variable), with a maximum magnitude of 2.84 and a minimum magnitude of
Canis_Minor
Binary star in the constellation Cepheus
Gamma Cephei, Iota Draconis, Theta Draconis, Eta Draconis, Zeta Draconis, Upsilon Draconis, 73 Draconis and 23 Cassiopeiae. A planet orbiting Gamma Cephei
Gamma_Cephei
Star in the constellation Capricornus
variations showing a phase cycle of 1.03 days. It is classified as a Gamma Cassiopeiae variable with an amplitude of 0.16 in magnitude. Epsilon Capricorni Aa
Epsilon_Capricorni
Star in the constellation Canis Major
their search for beta Cephei variable stars in the southern sky. Christoffel Waelkens et al. confirmed that HR 2501 is variable in 1983, and reported that
HR_2501
Star in the constellation Canis Major
about 3.7 times the radius of the star. It is classified as a Gamma Cassiopeiae type variable star and its brightness varies from magnitude +3.4 to +3.97
Kappa_Canis_Majoris
Star in the constellation Crux
literature. Samus et al. (2017) have tentatively classified it as a Gamma Cassiopeiae variable with a brightness range of 4.88–5.7 mag in the Johnson B band
CH_Crucis
Star in the constellation Carina
the discovery that this star is a variable star, in 1951. This star is classified as a Gamma Cassiopeiae-type variable and its brightness varies from magnitude
PP_Carinae
Binary star system in the constellation Pisces
a weak magnetic field with a strength of 0.4±0.2 G, and is a Gamma Cassiopeiae variable. The companion, component B, is a magnitude 7.51 star. van Leeuwen
Eta_Piscium
Binary star system in the constellation Draco
designation HD 174237 in the Henry Draper Catalogue; CX Draconis is the variable star designation. This is a double-lined spectroscopic binary system with
CX_Draconis
Type of variable star
Catalogue of Variable Stars does not have a type for λ Eridani variables, only GCAS for Gamma Cassiopeiae variables and BE for non-GCAS Be star variables. λ Eridani
Lambda_Eridani_variable
Overview of the scientific field of astronomy
supergiants Luminous blue variable Gamma Cassiopeiae variable R Coronae Borealis variable Eruptive binary RS Canum Venaticorum variable Cataclysmic or explosive
Outline_of_astronomy
Star in the constellation Canis Major
Southern Hemisphere, Omega Canis Majoris is classified as a Gamma Cassiopeiae-type variable star. Both the luminosity and the radial velocity vary with
Omega_Canis_Majoris
Variable star in the constellation Lacerta
It is a Gamma Cassiopeiae variable, varying in brightness from magnitude 5.22 to 5.48, over a period of about 8.7 hours. The star's variable spectrum
EW_Lacertae
Variable star in the constellation Perseus
surrounded by a disk of expelled material. This qualifies it as a Gamma Cassiopeiae variable, and the visual range is magnitude 6 - 7. In 1989 and 1990, the
X_Persei
Star in the constellation Pavo
hot blue star which has developed a gas disk around it. It is a γ Cassiopeiae variable or shell star which has occasionally brightened to magnitude 4.0
Lambda_Pavonis
Open cluster in Puppis
5th magnitude stars are all variables: NV Puppis is a Gamma Cassiopeiae variable, while NW Puppis is a Beta Cephei variable. "Cl Collinder 135". SIMBAD
Collinder_135
Star in the constellation Sagittarius
It was given its variable star designation, V4024 Sagittarri, in 1978. It is classified as an eruptive Gamma Cassiopeiae variable and has been measured
V4024_Sagittarii
B-type star in the constellation Vulpecula
HD 192685 varies slightly in brightness and is classified as a γ Cassiopeiae variable. The stellar components have a projected separation of 70 astronomical
HD_192685
Star in the constellation Perseus
published in 1712. 48 Persei is classified as a Gamma Cassiopeiae variable, and it has been given the variable star designation MX Persei. The star's brightness
48_Persei
Star in the constellation Ophiuchus
66 Ophiuchi is a binary variable star in the equatorial constellation of Ophiuchus. It has the variable star designation V2048 Ophiuchi, while 66 Ophiuchi
66_Ophiuchi
Star in the constellation Circinus
magnitude, mass, and classification. The system behaves as a Gamma Cassiopeiae variable showing occasional outbursts of up to 0.27 in magnitude. "Hipparcos
Theta_Circini
Blue-hued variable star in the constellation Carina
with possible periods of 100 and 971 days. It is classified as a γ Cassiopeiae variable. V518 Carinae is classified as a B-type main sequence star between
V518_Carinae
Variable B-type star in the constellation Aquarius
effective temperature of 11,145 K. This is classified as a Gamma Cassiopeiae type variable star and its brightness varies from magnitude +4.68 down to
Omicron_Aquarii
Star in the constellation Aquarius
lines) into an ordinary B-type star. It is classified as a Gamma Cassiopeiae type variable star and its brightness varies from magnitude +4.45 to +4.71;
Pi_Aquarii
Variable star in the constellation Centaurus
experience transient periodicities. Mu Centauri is classified as a Gamma Cassiopeiae type variable star and its brightness varies from magnitude +2.92 to +3.49
Mu_Centauri
Star in the constellation Ophiuchus
angle of its poles must be small; estimated as ~20°. It is a Gamma Cassiopeiae variable with an amplitude of 0.15 magnitude. The brightness has been measured
Chi_Ophiuchi
Star in the constellation Carina
to 4.52 in visual magnitude, and it has been classified as a Gamma Cassiopeiae variable. The star is 32 million years old and is spinning with a projected
V344_Carinae
Star in the constellation Orion
Orionis is a Gamma Cassiopeiae variable star, and has been given the variable star designation V1086 Orionis. The General Catalog of Variable Stars lists
25_Orionis
Star in the constellation Centaurus
It is also a variable star whose brightness varies from magnitude +2.51 to +2.65. It has been classified as a γ Cassiopeiae type variable. The energy from
Delta_Centauri
Constellation in the southern celestial hemisphere
variation can be observed with the unaided eye. Classed as a Gamma Cassiopeiae variable or shell star, it is of spectral type B2II-IIIe and lies around
Pavo_(constellation)
Binary star system in the constellation Canis Major
39 secondary, component B, is classified as a Gamma Cassiopeiae type variable star. Due to its variable nature, the brightness of the system varies from
27_Canis_Majoris
Variable star in the constellation Orion
1000 times that of the Earth. Omega Orionis is, like many Be stars, a variable star whose brightness varies 0.19 magnitudes. Also, small variations have
Omega_Orionis
Star in the constellation Cygnus
x, S2CID 14878976. Samus, N. N.; et al. (2017), "General Catalogue of Variable Stars", Astronomy Reports, GCVS 5.1, 61 (1): 80–88, Bibcode:2017ARep..
59_Cygni
Star in the constellation Camelopardalis
designation in 1987. Samus et al. (2017) classify it as a Be variable, rather than a Gamma Cassiopeiae type, and it ranges from a peak Hipparcos magnitude of
11_Camelopardalis
Variable star in the constellation of Andromeda
Andromedae is a Gamma Cassiopeiae type variable star and the system's brightness varies from magnitude +3.58 to +3.78. The variable component is the
Omicron_Andromedae
Difference of intensity of the stellar continuum spectrum
Strecker, D. W. (1978). "Infrared excesses in early-type stars - Gamma Cassiopeiae". Astrophysical Journal. 224: 527. Bibcode:1978ApJ...224..527S. doi:10
Balmer_jump
Star in the constellation Apus
velocity along the equator. Epsilon Apodis is classified as a Gamma Cassiopeiae type variable star and its brightness varies between magnitudes 4.99 and
Epsilon_Apodis
Star in the constellation Cassiopeia
It was given the variable star designation V615 Cassiopeiae. LS I +61 303 emits HE and VHE (High Energy and Very High Energy) gamma rays. It is only one
LS_I_+61_303
Star in the constellation Perseus
match any particular orbital phase. The variations are classified as γ Cassiopeiae-type, shell stars with eruptions and irregular fading. Roman, Nancy G
Phi_Persei
Binary star system in the constellation Aquila
V923 Aquilae is a variable binary star system in the equatorial constellation of Aquila. It has the designation HD 183656 from the Henry Draper Catalogue;
V923_Aquilae
Star in the constellation Carina
constellation Carina. It has the Bayer designation E Carinae; V345 Carinae is the variable star designation. The star has a blue-white hue and is faintly visible
V345_Carinae
Star in the constellation Perseus
period 1.021 days. The General Catalog of Variable Stars classifies Psi Persei as a gamma Cassiopeiae variable star, whose visual band brightness varies
Psi_Persei
Variable Star in constellation Canis Major
its main-sequence life. It is a Be star and also a Gamma Cassiopeiae variable, eruptive variables that show irregular variations in their luminosity caused
FR_Canis_Majoris
Star in the constellation Pegasus
massive Be star with a stellar classification of B2IV-V. It is a γ Cas variable; a type of shell star with a circumstellar disc of gas surrounding the
31_Pegasi
Star in the constellation Puppis
is approximately 800 light years away based on parallax. It is a γ Cas variable, ranging from 4.78 to 4.58 magnitude. It is most likely an optical double
NV_Puppis
Star in the constellation Apus
shows some peculiarity in the spectrum. It is classified as a Gamma Cassiopeiae type variable star and its brightness varies from magnitude +5.43 to +5.61
Kappa1_Apodis
Nova in the constellation Cassiopeia seen in 2021
Nova Cassiopeiae began a linear decline in brightness. This nova has been detected throughout the electromagnetic spectrum, from radio to gamma rays.
Nova_Cassiopeiae_2021
Binary star system in the constellation Centaurus
circumstellar disk of decreated gas. It is classified as a suspected Gamma Cassiopeiae type variable star with a visual magnitude varying from +4.30 down to +4
HD_102776
there are over 52,011 known variable stars, with more being discovered regularly, so a complete list of every single variable is impossible at this place
List_of_variable_stars
Star naming system
1600. Tycho's Star (SN 1572), another "temporary star", appears as B Cassiopeiae. In charts for constellations that did not exhaust the Greek letters
Bayer_designation
which were references to the three Apollo 1 crew: Navi for the star Gamma Cassiopeiae and which is Ivan spelled backwards, the middle name of Virgil Ivan
Stars_named_after_people
Open star cluster in the constellation Cassiopeia
open cluster NGC 637, and the bright magnitude +2.2 irregular variable star Gamma Cassiopeiae. The cluster is 7 arcmins across. It was discovered by William
NGC_559
Small number of stars that orbit each other
the system can be considered a sextuple. Jabbah AR Cassiopeiae V871 Centauri Acrux Gamma Cassiopeiae QZ Carinae Astronomy portal Outer space portal Science
Star_system
Zodiac constellation in the southern celestial hemisphere
is a shell star of magnitude 4.9. Shell stars, like Pleione and Gamma Cassiopeiae, are stars with irregular variations caused by their abnormally high
Libra_(constellation)
Classification of stars based on spectral properties
sources are marked by a letter beta (β) for intermediate surface gravity and gamma (γ) for low surface gravity. Indication for low surface gravity are weak
Stellar_classification
E. N. (2009-01-01). "VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+, 2007-2017)". VizieR Online Data Catalog: B/gcvs. Bibcode:2009yCat
List of brightest natural objects in the sky
List_of_brightest_natural_objects_in_the_sky
Constellation split into two non-contiguous parts
AAVSO Website. American Association of Variable Star Observers. Retrieved 22 May 2014. "* Gamma Serpentis – Variable star". SIMBAD. Retrieved 22 May 2014
Serpens
cluster GCAS – (celestial object) Gamma CASsiopeiae, a class of eruptive variable stars named after Gamma Cassiopeiae, the archetype for the class GCMS
List_of_astronomy_acronyms
ul-Khaḍib the Palm (reaching from the Pleiades) الكـــف الخضيب Beta Cassiopeiae Celbalrai Kalb ur-Rāʿī the Shepherd's Dog كلب الراعي Beta Ophiuchi Chertan
List_of_Arabic_star_names
System of two stars orbiting each other
binary white dwarf system with an orbital period of about 5.4 minutes Eta Cassiopeiae, a nearby visual binary star system in the constellation Cassiopeia Kepler-14
Binary_star
(2011-05-10). "Colder and Hotter: Interferometric imaging of {\beta} Cassiopeiae and {\alpha} Leonis". The Astrophysical Journal. 732 (2): 68. arXiv:1105
List_of_nearest_giant_stars
Astrophysical phenomenon
Betelgeuse, Antares, and VV Cephei A; the yellow hypergiant Rho Cassiopeiae; the luminous blue variable Eta Carinae that has already produced a supernova impostor;
Supernova
IanRidpath.com. "Cujam". stars.astro.illinois.edu. Retrieved 2026-04-07. "Gacrux/Gamma Crucis 2?". Sol Station. Sol Company. Archived from the original on 2011-11-03
List_of_proper_names_of_stars
Prominent examples of stars in this mass range include Antares, Spica, Gamma Velorum, Mu Cephei, and members of the Quintuplet Cluster. Type Ia supernova
List_of_supernova_candidates
supernovae List of supernova candidates List of supernova remnants List of gamma-ray bursts List of most distant supernovae Table of stars with Bayer designations
Lists_of_stars
Star in the constellation Crux
variable star of the Gamma Cassiopeiae type, indicating it is a shell star with a circumstellar disk of gas about the equator, and has the variable star
HD_110432
Constellation in the northern celestial hemisphere
N. (1982). "A Comparison of the X-ray Properties of X Persei and Gamma Cassiopeiae". The Astrophysical Journal. 263 (1): 277–88. Bibcode:1982ApJ...263
Perseus_(constellation)
Star in the constellation Columba
equatorial velocity may be 457 km s−1. It is a suspected Gamma Cassiopeiae type (GCAS) variable star, with its apparent magnitude varying from 2.62m to
Alpha_Columbae
Vols I-III and NL 67-78 with improved coordinates, General Catalogue of Variable Stars Archived 2017-06-20 at the Wayback Machine, Sternberg Astronomical
List of star systems within 150–200 light-years
List_of_star_systems_within_150–200_light-years
Star in the constellation Draco
General Catalogue of Variable Stars lists Kappa Draconis as a Gamma Cassiopeiae type star, a type of eruptive irregular variable star, whose visual magnitude
Kappa_Draconis
Type of variable star
to as rapidly oscillating α2 Canum Venaticorum variables. Both the roAp stars and some α2 CVn variables lie on the δ Scuti instability strip and are magnetic
Rapidly_oscillating_Ap_star
Star system in the constellation of Telescopium
Catalogue of Variable stars includes this system as a variable similar to but not properly of the Gamma Cassiopeiae type, with the variable star designation
HR_6819
Variable star in the constellation Hercules
just left the main sequence. Omicron Herculis is an eruptive variable of the Gamma Cassiopeiae class, which are rapidly rotating B-class stars with mass
Omicron_Herculis
Brightest star in the constellation Leo
Sturmann, L. (2011-04-18). "Colder and Hotter: Interferometric imaging of β Cassiopeiae and α Leonis". The Astrophysical Journal. 732 (2): 68. arXiv:1105.0740
Regulus
"Hubble Space Telescope Astrometry of the Metal-poor Visual Binary μ Cassiopeiae: Dynamical Masses, Helium Content, and Age". The Astrophysical Journal
List of nearest stars by spectral type
List_of_nearest_stars_by_spectral_type
Stars sorted by absolute magnitude
Way. (Note that quasars often vary somewhat in luminosity.) In terms of gamma rays, a magnetar (type of neutron star) called SGR 1806−20, had an extreme
List_of_most_luminous_stars
Star in the constellation Canis Major
oxygen-rich red hypergiant or red supergiant (O-rich RHG or RSG) and pulsating variable star 1.2 kiloparsecs (3,900 light-years) from the Solar System in the slightly
VY_Canis_Majoris
Class of high-mass X-ray binaries
optical counterparts. X Persei is a binary system containing a γ Cassiopeiae variable and a pulsar. It has a relatively long period and low eccentricity
Be/X-ray_binary
GAMMA CASSIOPEIAE-VARIABLE
GAMMA CASSIOPEIAE-VARIABLE
Girl/Female
Gujarati, Hindu, Indian
The Soothing Voice
Girl/Female
African, American, Australian, British, Chinese, Christian, Danish, Dutch, English, French, German, Irish, Italian, Jamaican, Latin
Jewel; Precious Stone; Gem
Female
English
Italian name GEMMA means "precious stone."
Boy/Male
Arabic
Two Bright Stars Near the Pole; Beta and Gama in Ursa Minor
Girl/Female
Tamil
Beautiful, A destiny
Male
Greek
(ΚηφεÏÏ‚) Greek name KEPHEUS means "gardener." In mythology, this is the name of a king of Ethiopia, the husband of Kassiopeia.
Surname or Lastname
English
English : variant of Game.English : from Anglo-Norman French gambon ‘ham’, a diminutive of gambe, Norman-Picard form of Old French jambe ‘leg’ (Late Latin gamba), hence probably a nickname for someone with some peculiarity of the legs or gait.
Boy/Male
Indian
Supreme god.
Boy/Male
African, British, English, Indian
Mother; God-like
Girl/Female
Arabic, Indian, Kashmiri
Beautiful Sky
Female
Greek
(ΚασσιÎπεια) Greek name KASSIOPEIA means "she whose words excel." In mythology, this is the name of one of the fifty Nereids who became the wife of Kepheus and mother of AndromÄ“de.Â
Girl/Female
Norse
Grandmother.
Girl/Female
Hindu, Indian, Kannada, Telugu
Beautiful; A Destiny
Girl/Female
Greek
Mother of Andromeda.
Girl/Female
Australian, French, Hebrew
Without Flaw; Palm Tree; Perfect
Girl/Female
Arabic
Variant of Cassiopeia
Girl/Female
Hebrew
Without flaw.
Female
English
Variant spelling of Italian Gemma, JEMMA means "precious stone."
Girl/Female
French Latin Italian
Jewel.
Girl/Female
Danish, Indian, Latin, Sanskrit, Swedish
Loveable; Desire
GAMMA CASSIOPEIAE-VARIABLE
GAMMA CASSIOPEIAE-VARIABLE
Boy/Male
Teutonic American German
Mighty horse.
Boy/Male
British, English, Irish
Son of Cunotamus
Male
Egyptian
, the royal scribe of an unnamed monarch.
Male
Babylonian
, the father of Nabu-salim.
Girl/Female
Hindu, Indian, Sanskrit, Tamil
Worshipper of Vishnu; Goddess is Vaishno Devi
Boy/Male
Tamil
Jayasankar | ஜயாஸஂகரÂ
Lord Krishna
Boy/Male
Hindu
Excellent
Male
English
Short form of Welsh Dylan, DYL means "great sea."
Girl/Female
Biblical
The praise of the Lord.
Girl/Female
Hindu, Indian, Marathi
Courageous
GAMMA CASSIOPEIAE-VARIABLE
GAMMA CASSIOPEIAE-VARIABLE
GAMMA CASSIOPEIAE-VARIABLE
GAMMA CASSIOPEIAE-VARIABLE
GAMMA CASSIOPEIAE-VARIABLE
n.
A constellation of the northern hemisphere, situated between Cepheus and Perseus; -- so called in honor of the wife of Cepheus, a fabulous king of Ethiopia.
a.
Belonging to, or resembling, gumma.
n.
A glandular organ for secreting milk, characteristic of all mammals, but usually rudimentary in the male; a mammary gland; a breast; under; bag.
pl.
of Gumma
pl.
of Gemma
n.
A child's name for mamma, mother.
n.
Mamma.
n.
The llama.
n.
A viola da gamba.
n.
A kind of soft tumor, usually of syphilitic origin.
n.
A bud spore; one of the small spores or buds in the reproduction of certain Protozoa, which separate one at a time from the parent cell.
n.
A leaf bud, as distinguished from a flower bud.
n.
See Mamma.
n.
Mother; -- word of tenderness and familiarity.
a.
Having the form of a mamma (breast) or mammae.
a.
Of or pertaining to a gumma.
pl.
of Mamma
n.
An abbes or spiritual mother.
n.
The viola di gamba, now entirely disused.
n.
The third letter (/, / = Eng. G) of the Greek alphabet.