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Optical interferometer on Mount Wilson, California
The CHARA (Center for High Angular Resolution Astronomy) array is an optical interferometer, located on Mount Wilson, California. The array consists of
CHARA_array
Astronomical observatory in Los Angeles County, California, US
in 1908, the 150-foot (46 m) solar tower completed in 1912, and the CHARA array, built by Georgia State University, which became fully operational in
Mount_Wilson_Observatory
Topics referred to by the same term
related to Chara. Chara (alga), a genus of algae in the family Characeae Chara (moth), a genus of moths in the family Noctuidae CHARA array, a telescope
Chara
Effective Temperatures of B-type Stars from Optical Interferometry with the CHARA Array". The Astrophysical Journal. 873 (1): 91. Bibcode:2019ApJ...873...91G
List of stars with resolved images
List_of_stars_with_resolved_images
Brightest star in the constellation Aquila
from 2006 infrared observations made with the MIRC instrument on the CHARA array interferometer; this was the first time the surface of any main-sequence
Altair
Brightest star in the constellation Lyra
2001 and then later confirmed with the CHARA array at Mt. Wilson in 2006 and the Infrared Optical Telescope Array at Mt. Hopkins in 2011, revealed evidence
Vega
F.; Thompson, R. R.; Coyne, J. (2006-01-20). "First Results from the CHARA Array. III. Oblateness, Rotational Velocity and Gravity Darkening of Alderamin"
List of nearest stars by spectral type
List_of_nearest_stars_by_spectral_type
Northern pole-star; brightest star in Ursa Minor
inner binary using the interferometric CHARA Array. They improved the solution of the orbit: combining CHARA data with previous Hubble data, and in tandem
Polaris
Mountain in California, United States
60-foot (18.3 m) and 150-foot (45.7 m) tall solar towers. The newer CHARA array, run by Georgia State University, is also sited there and does important
Mount_Wilson_(California)
Telescope in the Atacama Desert, Chile
the resolution achieved using other arrays such as the Navy Prototype Optical Interferometer and the CHARA array. Unlike many earlier optical and infrared
Very_Large_Telescope
2024). "The Orbit and Dynamical Mass of Polaris: Observations with the CHARA Array". The Astrophysical Journal. 971 (2): 190. arXiv:2407.09641. Bibcode:2024ApJ
List_of_largest_stars
Array used for astronomical observations
expected to produce their first images soon, including the VLTI, the CHARA array and Le Coroller and Dejonghe's Hypertelescope prototype. If completed
Astronomical_interferometer
Yellow hypergiant star in the constellation Cassiopeia
infrared. In 2023, Rho Cassiopeiae was imaged through interferometry at the CHARA array. The star was observed at the H and K near-infrared wavelengths, and
Rho_Cassiopeiae
Multiple star system in the constellation of Lyra
accretion disk of the secondary star were resolved and imaged using the CHARA Array interferometer and the Michigan InfraRed Combiner (MIRC) in the near
Beta_Lyrae
Brightest star in Earth's night sky
Aufdenberg, J.P.; Ridgway, S.T.; et al. (2006). "First results from the CHARA Array: VII. Long-Baseline Interferometric Measurements of Vega Consistent with
Sirius
synthesis soon,[needs update] followed by other interferometers such as the CHARA array and the Magdalena Ridge Observatory Interferometer which may consist
Astronomical optical interferometry
Astronomical_optical_interferometry
Public university in Atlanta, Georgia, US
Moderate Aperture Research Telescope System (or SMARTS) in Chile, and the CHARA array on Mount Wilson Observatory in Los Angeles County, California, Hard Labor
Georgia_State_University
Brightest star in the constellation Leo
Grundstrom; Ogden; Ridgway; Van Belle; et al. (2005). "First Results from the CHARA Array. I. An Interferometric and Spectroscopic Study of the Fast Rotator Alpha
Regulus
Extrasolar planet in the Andromeda constellation
not detected using high-resolution inferterometric observations by the CHARA array. Tidal heating models predict a similar mass for the planet. The planet
Upsilon_Andromedae_b
Hypergiant star in the constellation Cepheus
great dimming event, and it was subsequently observed by the CHARA interferometry array in December. The distance to RW Cephei has been estimated on the
RW_Cephei
other astronomical telescope arrays including: the Navy Prototype Optical Interferometer, the CHARA array, and the IOTA array. In 2008, Max Tegmark and Matias
History_of_the_telescope
Star in the constellation of Cepheus
parsecs or approximately 49 light years from Earth. Interferometry by the CHARA array show that Alderamin has an oblate shape, its equatorial size measures
Alpha_Cephei
Star system in the constellation Taurus
Sturmann, L.; Sturmann, J.; Turner, N. H.; Farrington, C. (2013). "A CHARA Array Survey of Circumstellar Disks around Nearby Be-type Stars". The Astrophysical
Alcyone_(star)
Star in the constellation Lacerta
main-sequence. It is the star with the smallest angular diameter measured by the CHARA array as of 2018[update], at 0.11±0.02 milliarcseconds. 10 Lacertae has an
10_Lacertae
Stellar classification
Riedel, Adric R.; Ireland, Michael; von Braun, Kaspar (2012-12-10). "The Chara Array Angular Diameter of Hr 8799 Favors Planetary Masses for ITS Imaged Companions"
A-type_main-sequence_star
Astronomical observatory network in southern France
(CERGA) Cote d'Azur Observatory tested beam combining technology at CHARA array. Astronomers developed a theory about M-Type asteroids, that may be tested
Côte_d'Azur_Observatory
Star system in the constellation Cassiopeia
DR3 record for this source at VizieR. Klement, R.; et al. (2024). "The CHARA Array Interferometric Program on the Multiplicity of Classical Be Stars: New
Gamma_Cassiopeiae
Star in the constellation of Draco
; et al. (June 2010). "Separated Fringe Packet Observations with the CHARA Array. I. Methods and New Orbits for χ Draconis, HD 184467, and HD 198084"
Chi_Draconis
Star in the constellation Draco
Sigma Draconis has been directly measured using interferometry with the CHARA array, which yields a result of 77.6% of the Sun's radius. It has 84% of the
Sigma_Draconis
Star in the constellation Pegasus
Effective Temperatures of B-type Stars from Optical Interferometry with the CHARA Array". The Astrophysical Journal. 873 (1): 91. Bibcode:2019ApJ...873...91G
Alpha_Pegasi
US Navy astronomical interferometer
also used to align the long train of optics. The NPOI siderostat array and the CHARA Array are the world's only long-baseline optical interferometers that
Navy Precision Optical Interferometer
Navy_Precision_Optical_Interferometer
Star in the constellation Pegasus
Adric R.; Ireland, Michael; von Braun, Kaspar (21 November 2012). "The CHARA Array Angular Diameter of HR 8799 Favors Planetary Masses for Its Imaged Companions"
HR_8799
Historically black university in Savannah, Georgia, US
Southern Polytechnic State University Waycross College Research GSU CHARA array Hard Labor Creek Observatory Georgia Tech ATDC IRIM GTRC GTRI Nanotechnology
Savannah_State_University
Five-star system in the constellation Orion
components of σ Orionis A have been resolved interferometrically using the CHARA array, and the combination of interferometric and visual observations yields
Sigma_Orionis
Star in the constellation Virgo
S. T.; Aufdenberg, J. P.; Merand, A. (2006), "First Results from the CHARA Array. IV. The Interferometric Radii of Low-Mass Stars", The Astrophysical
Gliese_514
Star in the constellation Lyra
Effective Temperatures of B-type Stars from Optical Interferometry with the CHARA Array". The Astrophysical Journal. 873 (1): 91. Bibcode:2019ApJ...873...91G
Gamma_Lyrae
and limb darkening of the asteroseismic red giant η Serpentis with the CHARA Array". Astronomy and Astrophysics. 517: A64. Bibcode:2010A&A...517A..64M.
List_of_nearest_giant_stars
Binary star in the constellation Draco
Effective Temperatures of B-type Stars from Optical Interferometry with the CHARA Array", The Astrophysical Journal, 873 (1): 91, Bibcode:2019ApJ...873...91G
Zeta_Draconis
Triple star system in the constellation Aquila
determined using interferometry at the Very Large Telescope and the CHARA array, the average of both measurements, combined with its estimated distance
Beta_Aquilae
Star in the constellation Perseus
SU Persei was imaged by the CHARA array in 2015, 2016, 2019, 2020, and 2021. Observations during 2015 and 2016 with CHARA show that the star has an angular
SU_Persei
Constellation in the northern celestial hemisphere
Spectroscopic Binary σ2 Coronae Borealis from Interferometry at the Chara Array". The Astrophysical Journal. 690 (1): 394–406. arXiv:0808.4015. Bibcode:2009ApJ
Corona_Borealis
Georgia State University for adaptive optics upgrade on telescopes at CHARA array. 2015 ALPAO released the DM468 and the DM820. 2013 ALPAO released the
ALPAO
American astronomer
She studied the sizes of nearby stars similar to the Sun, using GSU's CHARA array, a long-baseline optical and infrared interferometer located at Mount
Tabetha_S._Boyajian
Star in the constellation Cygnus
Located 2,090 parsecs (6,800 ly) from Earth, it has been studied by the CHARA array in order to understand the surface variations of red supergiants. AZ
AZ_Cygni
Star in the constellation Orion
Effective Temperatures of O-type Stars from Optical Interferometry with the CHARA Array". The Astrophysical Journal. 869 (1): 37. arXiv:1812.05511. Bibcode:2018ApJ
Meissa
Star that is particularly similar to the Sun
Dwarfs s Draconis and HR 511 from Interferometric Measurements with the CHARA Array". The Astrophysical Journal. 683 (1): 424–432. arXiv:0804.2719. Bibcode:2008ApJ
Solar_analog
Star in the constellation Taurus
Effective Temperatures of B-type Stars from Optical Interferometry with the CHARA Array". The Astrophysical Journal. 873 (1): 91. Bibcode:2019ApJ...873...91G
Beta_Tauri
Star in the constellation Hercules
Effective Temperatures of B-type Stars from Optical Interferometry with the CHARA Array". The Astrophysical Journal. 873 (1): 91. Bibcode:2019ApJ...873...91G
Iota_Herculis
Star in the constellation Draco
"Fundamental Parameters of the Exoplanet Host K Giant Star ι Draconis from the CHARA Array", The Astrophysical Journal, 743 (2): 130, arXiv:1109.4950, Bibcode:2011ApJ
Iota_Draconis
Archived from the original on 7 December 2018. Retrieved 27 July 2018. "CHARA Array". "Contacts - astrosat". astrosat.iucaa.in. "SPARCS". Evgenya Shkolnik
List of women in leadership positions on astronomical instrumentation projects
List_of_women_in_leadership_positions_on_astronomical_instrumentation_projects
Red-clump giant star in the constellation Aquila
stellar companion can be ruled out based upon observations with the CHARA array. In 2008, the presence of a planetary companion was announced, based
Xi_Aquilae
Binary star system in the constellation Pisces
Ba-Bb Subsystem in α Piscium: First Dual-Field Interferometry at the CHARA Array", The Astronomical Journal, arXiv:2603.09489. Gray, R. O.; Garrison,
Alpha_Piscium
Multiple star in the constellation Taurus
years. The angular diameter of this star has been measured using the CHARA array to 2% accuracy. After correcting for limb darkening, this gives the stellar
Gamma_Tauri
Binary star system
Dwarfs σ Draconis and HR 511 from Interferometric Measurements with the CHARA Array". The Astrophysical Journal. 683 (1): 424–432. arXiv:0804.2719. Bibcode:2008ApJ
Mu_Cassiopeiae
Star in the constellation Cepheus
Effective Temperatures of B-type Stars from Optical Interferometry with the CHARA Array". The Astrophysical Journal. 873 (1): 91. Bibcode:2019ApJ...873...91G
Beta_Cephei
letters. T.A. ten Brummelaar; et al. (2005). "First Results from the CHARA Array. II. A Description of the Instrument". Astrophysical Journal. 628 (1):
List of astronomical interferometers at visible and infrared wavelengths
List_of_astronomical_interferometers_at_visible_and_infrared_wavelengths
Multiple star system in the constellation of Auriga
like a 550 K black body. The 2009–2011 eclipse was well observed and CHARA array was able to directly image the shape of the disk in a silhouette. The
Epsilon_Aurigae
(2024-08-01). "The Orbit and Dynamical Mass of Polaris: Observations with the CHARA Array". The Astrophysical Journal. 971 (2): 190. arXiv:2407.09641. Bibcode:2024ApJ
List_of_nearest_supergiants
Spectroscopic binary star in the constellation Hercules
long baseline interferometry. Interferometric observations from the CHARA Array enabled its three dimensional orbit with a semimajor axis of 2.01 ± 0
AC_Herculis
Star in the constellation Auriga
optical companions. A new potential companion was discovered using the CHARA array in 2023. In December 2017, it had an angular separation from AE Aurigae
AE_Aurigae
Star in the constellation Draco
ISSN 0004-637X. Berger, D. H.; et al. (2006). "First Results from the CHARA Array. IV. The Interferometric Radii of Low-Mass Stars". The Astrophysical
Gliese_687
Star in the constellation Pegasus
Effective Temperatures of B-type Stars from Optical Interferometry with the CHARA Array". The Astrophysical Journal. 873 (1): 91. Bibcode:2019ApJ...873...91G
Zeta_Pegasi
Star in the constellation Aries
Effective Temperatures of B-type Stars from Optical Interferometry with the CHARA Array", The Astrophysical Journal, 873 (1): 91, Bibcode:2019ApJ...873...91G
Gamma_Arietis
Star in the constellation Pisces
angular diameter has been directly determined by interferometry using the CHARA array, yielding a true radius 85% of the Sun's radius. The rotational period
54_Piscium
Binary star system in the constellation Aquila
V.; et al. (2022), "Visual Orbits of Spectroscopic Binaries with the CHARA Array. IV. HD 61859, HD 89822, HD 109510, and HD 191692", The Astronomical
Theta_Aquilae
Multiple star in the constellation Cygnus
N. H (2013). "Interferometric radii of bright Kepler stars with the CHARA Array: θ Cygni and 16 Cygni a and B". Monthly Notices of the Royal Astronomical
16_Cygni
Star in the constellation Ursa Major
"Angular Diameters and Effective Temperatures of 25 K Giant Stars from the CHARA Array". Astrophysical Journal. 710 (2): 1365–1374. arXiv:0912.5491. Bibcode:2010ApJ
4_Ursae_Majoris
Star in the constellation Leo
Effective Temperatures of B-type Stars from Optical Interferometry with the CHARA Array". The Astrophysical Journal. 873 (1): 91. Bibcode:2019ApJ...873...91G
Sigma_Leonis
Star in the constellation Gemini
"Ruling Out Possible Secondary Stars to Exoplanet Host Stars Using the CHARA Array". The Astronomical Journal. 140 (1): 167–176. arXiv:1005.2930. Bibcode:2010AJ
HD_50554
Star in the constellation Auriga
has not been confirmed. The strongest evidence was found in 2013 using CHARA array optical interferometry. The companion would be 6.7 magnitudes fainter
RT_Aurigae
Star in the constellation Sextans
H.; et al. (May 2018), "AB Dor Moving Group Stars Resolved with the CHARA Array", The Astrophysical Journal, 858 (2): 14, Bibcode:2018ApJ...858...71S
Gliese_393
American astronomer (born 1968)
in the commissioning of the Palomar Testbed Interferometer, and the CHARA Array. In 2007, he became a member of the astronomy faculty at the European
Gerard_van_Belle
Third-magnitude star in the constellation Cygnus
Effective Temperatures of B-type Stars from Optical Interferometry with the CHARA Array". The Astrophysical Journal. 873 (1): 91. Bibcode:2019ApJ...873...91G
Delta_Cygni
Star in the constellation Cetus
signature was confirmed using the separated fringe packet technique with the CHARA array. It is most likely a K-type main-sequence star with a class of K3.5 V
13_Ceti
Angular motion of a star about its axis
H. A.; ten Brummelaar, T. A.; et al. (2005). "First Results from the CHARA Array. I. An Interferometric and Spectroscopic Study of the Fast Rotator Alpha
Stellar_rotation
Star in the constellation Cepheus
C. D.; et al. (2014). "Separated Fringe Packet Observations with the CHARA Array. II. omega Andromeda, HD 178911, and xi Cephei". The Astronomical Journal
Xi_Cephei
Spectroscopic binary star system in the constellation Perseus
0.6. It has also been spatially resolved with interferometry at the CHARA array. There are distant companions B (separation 75.5" and magnitude 10.66)
43_Persei
Double star system in the constellation Camelopardalis
early B class subgiant. An additional star was discovered using the CHARA array, and has a mean separation from 1 Camelopardalis A of 26.16 mas. There
1_Camelopardalis
Star in the constellation Aquila
Effective Temperatures of B-type Stars from Optical Interferometry with the CHARA Array", The Astrophysical Journal, 873 (1): 91, Bibcode:2019ApJ...873...91G
Lambda_Aquilae
Star in the constellation Serpens
and limb darkening of the asteroseismic red giant η Serpentis with the CHARA Array", Astronomy and Astrophysics, 517: A64, Bibcode:2010A&A...517A..64M,
Eta_Serpentis
Variable star in the constellation Ursa Major
Ursae Majoris was measured in red light during 2015 and 2016, using the CHARA array. The limb darkened angular diameter was 0.226±0.008 milliarcseconds.
84_Ursae_Majoris
Star in the constellation of Cygnus
Gordon, Kathryn; Pablo, Herbert; Ramiaramanantsoa, Tahina (2016). "The CHARA Array resolves the long-period Wolf–Rayet binaries WR 137 and WR 138". Monthly
WR_137
Star in the constellation Cassiopeia
Effective Temperatures of B-type Stars from Optical Interferometry with the CHARA Array", The Astrophysical Journal, 873 (1): 91, Bibcode:2019ApJ...873...91G
Zeta_Cassiopeiae
Star in the constellation Corona Borealis
evolved intermediate-mass planet-hosting stars measured with PAVO at the CHARA Array". Monthly Notices of the Royal Astronomical Society. 477 (4): 4403–4413
Kappa_Coronae_Borealis
Star in the constellation Aquila
Effective Temperatures of B-type Stars from Optical Interferometry with the CHARA Array", The Astrophysical Journal, 873 (1): 91, Bibcode:2019ApJ...873...91G
Iota_Aquilae
Solitary star in the constellation Cassiopeia
The angular diameter of this star has been measured directly using the CHARA Array, yielding an estimate of 4.5 times the diameter of the Sun. Stellar models
HR_297
Star in the constellation Cetus
Effective Temperatures of B-type Stars from Optical Interferometry with the CHARA Array". The Astrophysical Journal. 873 (1): 91. Bibcode:2019ApJ...873...91G
Xi2_Ceti
Star in the constellation Corona Borealis
Spectroscopic Binary σ2 Coronae Borealis from Interferometry at the CHARA Array". The Astrophysical Journal. 690 (1): 394–406. arXiv:0808.4015. Bibcode:2009ApJ
Sigma_Coronae_Borealis
Star in the constellation Cygnus
with a radius around 850 R☉, measured by its angular diameter by the CHARA array. It is about 90,000 times more luminous that the Sun and has a cool effective
BI_Cygni
Star in the constellation Lyra
T. A. (October 2018). "Separated Fringe Packet Observations with the CHARA Array. III. The Very High-eccentricity Binary HR 7345". The Astronomical Journal
HD_181655
Star in the constellation Lynx
evolved intermediate-mass planet-hosting stars measured with PAVO at the CHARA Array". Monthly Notices of the Royal Astronomical Society. 477 (4): 4403–4413
6_Lyncis
Star in the constellation Cassiopeia
record for this source at VizieR. Touhami, Y.; et al. (May 2013). "A CHARA Array Survey of Circumstellar Disks around Nearby Be-type Stars". The Astrophysical
Omicron_Cassiopeiae
Star in the constellation Hercules
optical and near-IR wavelengths with the VLTI, NPOI, IOTA, PTI, and the CHARA Array". Astronomy & Astrophysics. 559: A111. arXiv:1308.6715. Bibcode:2013A&A
89_Herculis
Star in the constellation Coma Berenices
V.; et al. (2022), "Visual Orbits of Spectroscopic Binaries with the CHARA Array. IV. HD 61859, HD 89822, HD 109510, and HD 191692", The Astronomical
24_Comae_Berenices
Variable star in the constellation Hercules
Effective Temperatures of B-type Stars from Optical Interferometry with the CHARA Array", The Astrophysical Journal, 873 (1): 91, Bibcode:2019ApJ...873...91G
Tau_Herculis
Binary star system in the constellation of Leo
separation of 56.9 milliarcseconds between both components using the CHARA array. Both stars are completing one orbit around each other every 537 days
35_Leonis
Instrument mounted on the Very Large Telescope
papers had been published using AMBER data. Astronomical interferometer CHARA array GRAVITY – Very Large Telescope#Instruments Infrared Spatial Interferometer
AMBER_(Very_Large_Telescope)
1996 film
pop-singer Chara, and Ayumi Ito. The film was shot on hand-held cameras using jump cuts and other visual techniques. It covers a wide array of themes and
Swallowtail_Butterfly_(film)
astronomer at the Georgia State University. He is the Director of the CHARA Array and a leader in the development of the use of optical interferometry
Meanings of minor-planet names: 28001–29000
Meanings_of_minor-planet_names:_28001–29000
Star in the constellation Cygnus
(December 2019). "Visual Orbits of Spectroscopic Binaries with the CHARA Array. II. The Eclipsing Binary HD 185912". The Astronomical Journal. 158 (6):
HR_7484
CHARA ARRAY
CHARA ARRAY
Girl/Female
Indian
Dhara
Girl/Female
Tamil
Dhara
Female
Hebrew
(חַוָּה) Variant spelling of Hebrew Chavva, CHAVA means "life."Â
Female
Greek
(ΧαÏά) Greek name derived from the word chara, CHARA means "joyful."
Female
Spanish
Pet form of Spanish Rosario, CHARO means "rosary."
Female
English
Feminine form of Latin Clarus, CLARA means "clear, bright." In use by the English and Italians.
Female
English
Anglicized form of Irish Gaelic Ciara, CEARA means "little black one."
Boy/Male
Muslim
Charm
Girl/Female
African, Indian, Swahili
Charm
Female
Hebrew
Variant spelling of Hebrew Channa, CHANA means "favor; grace."Â
Girl/Female
African, Bengali, French, Gujarati, Hindu, Indian, Italian, Kannada, Latin, Malayalam, Sanskrit
Quiet and Frisky; Option; Happiness; Joy
Female
Italian
Italian form of Latin Clara, CHIARA means "clear, bright."
Female
English
Modern English name derived either from Italian cara, a term of endearment CARA means "beloved," or from the Irish Gaelic word cara, meaning "friend."
Girl/Female
Irish
The feminine form of Ciaran, from the Irish ciar meaning “dark†and implies “dark hair and brown eyes.†St. Ciara was a distinguished seventh-century figure who established a monastery at Kilkeary in County Tipperary. It was the fourth most popular baby girl name in Ireland in 2003.
Girl/Female
Indian
Quiet and frisky
Female
Hebrew
(×—Ö·×™Ö¼Ö´×”) Feminine form of Hebrew Chayim, CHAYA means "alive."
Boy/Male
Indian
Charm
Surname or Lastname
English
English : habitational name from Chard or South Chard in Somerset, recorded in Domesday Book as Cerdren, possibly from Old English ceart ‘rough heathland’ + ærn ‘building’, ‘dwelling’. In some instances the surname may have arisen simply as a topographic name from ceart.French : from the personal name Chard, a short form of Richard;French : habitational name for someone from Chard in the department of Creuse.
Female
Irish
Feminine form of Irish Gaelic Ciarán, CIARA means "little black one."
Female
English
Pet form of English Charlene, CHARLA means "man."
CHARA ARRAY
CHARA ARRAY
Boy/Male
Australian, British, English, German
Following Thor; The God of Thunder
Girl/Female
Tamil
Sweet girl, Variant of donald great chief
Girl/Female
Indian, Telugu
Parents Gift; Woman who has Lotus Like Wide Eyes
Girl/Female
Hindu, Indian
Name of Lord Vishnu
Boy/Male
Arabic, Parsi
Leisure; Happiness; Opportunity
Boy/Male
Tamil
Girl/Female
Arabic, Australian, Bengali, Indian, Muslim
Solver; Cleanliness; Intelligent; Pure
Boy/Male
Spanish
Frenchman.
Girl/Female
Tamil
Flower
Boy/Male
Indian
Light of God Ganesha
CHARA ARRAY
CHARA ARRAY
CHARA ARRAY
CHARA ARRAY
CHARA ARRAY
pl.
of Char-a-bancs
n.
To burn slightly or partially; as, to char wood.
n.
A sheet of paper, pasteboard, or the like, on which information is exhibited, esp. when the information is arranged in tabular form; as, an historical chart.
imp. & p. p.
of Chark
v. t.
To lay down in a chart; to map; to delineate; as, to chart a coast.
n.
Alt. of Charr
v. t.
Alt. of Chare
p. pr. & vb. n.
of Charm
v. i.
Alt. of Chare
v. i.
To act as, or produce the effect of, a charm; to please greatly; to be fascinating.
a.
Sparing; chary.
n.
One of the several species of fishes of the genus Salvelinus, allied to the spotted trout and salmon, inhabiting deep lakes in mountainous regions in Europe. In the United States, the brook trout (Salvelinus fontinalis) is sometimes called a char.
v. t.
To burn to a coal; to char.
n.
A charter or deed; a writing by which a grant is made. See Magna Charta.
n. & v.
A chore; to chore; to do. See Char.
imp. & p. p.
of Chart
n.
See 1st Char.
imp. & p. p.
of Charm