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W Aquilae information


W Aquilae

W Aquilae showing the close companion
Credit: Hubble Legacy Archive
Observation data
Epoch J2000      Equinox J2000
Constellation Aquila
Right ascension 19h 15m 23.357s[1]
Declination −07° 02′ 50.33″[1]
Apparent magnitude (V) A: 7.0 - 14.6[2]
B:14.8 [3]
Characteristics
A
Evolutionary stage asymptotic giant branch[4]
Spectral type S6/6e[4] (S3,9e - S6,9e[2])
B−V color index +2.58[5]
Variable type Mira[2]
B
Evolutionary stage main sequence[4]
Spectral type F8/9[4]
Astrometry
Radial velocity (Rv)−18.0[6] km/s
Proper motion (μ) RA: 15.713[1] mas/yr
Dec.: 0.103[1] mas/yr
Parallax (π)2.6735 ± 0.1392 mas[1]
Distance1,220 ± 60 ly
(370 ± 20 pc)
Absolute magnitude (MV)A: −0.7 to +6.9[3]
B: +7.1[3]
Details
A
Mass1.04 - 3[4] M
Radius444[7][a] R
Luminosity7,500[8] L
Temperature2,800[7] K
B
Mass1.04 - 1.09[4] M
Temperature5,900 - 6,170[4] K
Other designations
W Aql, IRAS 19126-0708, TYC 5142-2895-1, 2MASS J19152335-0702503, AAVSO 1910-07, Gaia DR2 420492505899016640
Database references
SIMBADdata

W Aquilae (W Aql) is a variable star in the constellation of Aquila. It is a type of evolved star known as an S-type star. Due to its relatively close distance of 1,200 light-years (370 pc) and equatorial location, it is easy to observe and heavily studied.[9]

  1. ^ a b c d e Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv:2208.00211. Bibcode:2023A&A...674A...1G. doi:10.1051/0004-6361/202243940. S2CID 244398875. Gaia DR3 record for this source at VizieR.
  2. ^ a b c Cite error: The named reference gcvs was invoked but never defined (see the help page).
  3. ^ a b c Cite error: The named reference mayer was invoked but never defined (see the help page).
  4. ^ a b c d e f g Cite error: The named reference danilovich was invoked but never defined (see the help page).
  5. ^ Cite error: The named reference tycho2 was invoked but never defined (see the help page).
  6. ^ Cite error: The named reference gcrv was invoked but never defined (see the help page).
  7. ^ a b Wallstrom, S. H. J.; Danilovich, T.; Muller, H. S. P.; Gottlieb, C. A.; Maes, S.; Van de Sande, M.; Decin, L.; Richards, A. M. S.; Baudry, A.; Bolte, J.; Ceulemans, T.; De Ceuster, F.; de Koter, A.; Mellah, I. El; Esseldeurs, M. (December 6, 2023). "ATOMIUM: Molecular inventory of 17 oxygen-rich evolved stars observed with ALMA". Astronomy & Astrophysics. 681: A50. arXiv:2312.03467. doi:10.1051/0004-6361/202347632. ISSN 0004-6361.
  8. ^ Brunner, M.; Danilovich, T.; Ramstedt, S.; Marti-Vidal, I.; De Beck, E.; Vlemmings, W. H. T.; Lindqvist, M.; Kerschbaum, F. (2018). "Molecular line study of the S-type AGB star W Aquilae". Astronomy & Astrophysics. 617: A23. arXiv:1806.01622. doi:10.1051/0004-6361/201832724. S2CID 67754573.
  9. ^ Cite error: The named reference Danilovich2021 was invoked but never defined (see the help page).


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