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18 Andromedae

From Wikipedia, the free encyclopedia
Blue-hued star in the constellation Andromeda
18 Andromedae
Location of 18 Andromedae (circled)
Observation data
Epoch J2000      Equinox J2000
ConstellationAndromeda
Right ascension23h 39m 08.33195s[1]
Declination+50° 28′ 18.2328″[1]
Apparent magnitude (V)5.350[2]
Characteristics
Evolutionary stagemain sequence[3]
Spectral typeB9 Ve[4]
B−Vcolor index−0.110[2]
Astrometry
Radial velocity (Rv)+9.9±2.2[5] km/s
Proper motion (μ)RA: −17.222[1]mas/yr
Dec.: −1.739[1]mas/yr
Parallax (π)7.8893±0.1288 mas[1]
Distance413 ± 7 ly
(127 ± 2 pc)
Details
Mass3.09±0.06[3] M
Luminosity146.6+14.1
−12.9
[3] L
Surface gravity (log g)3.632±0.014[2] cgs
Temperature10,351±50[2] K
Rotational velocity (v sin i)183[3] km/s
Other designations
18 And,BD+49°4180,FK5 3897,HD 222304,HIP 116709,HR 8967,SAO 35642,PPM 42060[6]
Database references
SIMBADdata

18 Andromedae, abbreviated18 And, is a single[7]star in the northernconstellation ofAndromeda.18 Andromedae is theFlamsteed designation. It is visible to the naked eye with anapparent visual magnitude of 5.350.[2] The annualparallax shift of7.9 mas[1] can be used to estimate a distance of 413 light years. It is moving further from the Earth with a heliocentricradial velocity of +10 km/s.[5]

This is aB-type main-sequence star with astellar classification of B9 Ve,[4] where the 'e' notation indicates this is aBe star. Thestellar spectrum of 18 And displays anemission line in the hydrogenBrackett series due to a dense gaseous circumstellar envelope.[4] The star is spinning rapidly with aprojected rotational velocity of 183 km/s and has about three times themass of the Sun. It is radiating 147 times theSun's luminosity[3] from itsphotosphere at aneffective temperature of 10,351 K.[2]

References

[edit]
  1. ^abcdefBrown, A. G. A.; et al. (Gaia collaboration) (August 2018)."Gaia Data Release 2: Summary of the contents and survey properties".Astronomy & Astrophysics.616. A1.arXiv:1804.09365.Bibcode:2018A&A...616A...1G.doi:10.1051/0004-6361/201833051.
  2. ^abcdefSoubiran, Caroline; et al. (2016), "The PASTEL catalogue: 2016 version",Astronomy & Astrophysics,591: A118,arXiv:1605.07384,Bibcode:2016A&A...591A.118S,doi:10.1051/0004-6361/201628497,S2CID 119258214.
  3. ^abcdeZorec, J.; Royer, F. (2012), "Rotational velocities of A-type stars. IV. Evolution of rotational velocities",Astronomy & Astrophysics,537: A120,arXiv:1201.2052,Bibcode:2012A&A...537A.120Z,doi:10.1051/0004-6361/201117691,S2CID 55586789.
  4. ^abcGranada, A.; et al. (May 2010), "Simultaneous K- and L-band spectroscopy of Be stars: circumstellar envelope properties from hydrogen emission lines",The Astronomical Journal,139 (5):1983–1992,Bibcode:2010AJ....139.1983G,doi:10.1088/0004-6256/139/5/1983,hdl:11336/9567.
  5. ^abGontcharov, G. A. (November 2006), "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system",Astronomy Letters,32 (11):759–771,arXiv:1606.08053,Bibcode:2006AstL...32..759G,doi:10.1134/S1063773706110065,S2CID 119231169.
  6. ^"18 And".SIMBAD.Centre de données astronomiques de Strasbourg. RetrievedSeptember 20, 2018.
  7. ^Eggleton, P. P.; Tokovinin, A. A. (September 2008), "A catalogue of multiplicity among bright stellar systems",Monthly Notices of the Royal Astronomical Society,389 (2):869–879,arXiv:0806.2878,Bibcode:2008MNRAS.389..869E,doi:10.1111/j.1365-2966.2008.13596.x,S2CID 14878976.
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