V Aquilae
Location of V Aquilae (circled) | |
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Aquila |
| Right ascension | Template:RA[1] |
| Declination | Template:DEC[1] |
| Apparent magnitude (V) | 6.6 - 8.4[2] |
| Characteristics | |
| Evolutionary stage | AGB[3] |
| Spectral type | C5,4-C6,4(N6)[2] |
| B−V color index | +4.32[4] |
| Variable type | SRb[2] |
| Astrometry | |
| Radial velocity (Rv) | +37[5] km/s |
| Proper motion (μ) | RA: 6.243±0.407[6] mas/yr Dec.: −1.379±0.318[6] mas/yr |
| Parallax (π) | 2.4779±0.2320 mas[6] |
| Distance | Template:Rnd ± Template:Rnd ly (Template:Rnd ± Template:Rnd pc) |
| Absolute magnitude (MV) | −5.19[7] |
| Details | |
| Mass | 2.5[8] M☉ |
| Radius | 234[9] R☉ |
| Luminosity | 6,500[10] L☉ |
| Surface gravity (log g) | −0.108[9] cgs |
| Temperature | 2,800[10] K |
| Metallicity [Fe/H] | 0.10[11] dex |
| Other designations | |
| BD−05 4858, HD 177336, HIP 93666, HR 7220, SAO 142985[12] | |
| Database references | |
| SIMBAD | data |
V Aquilae (V Aql) is a carbon star and semiregular variable star in the constellation Aquila. It has an apparent magnitude which varies between 6.6 and 8.4 and is located around 400 parsecs (1,300 ly) away.
V Aquilae is a type of star with a spectrum that is dominated by strong absorption lines of the molecules C2 and CN, hence known as carbon stars. The enhanced levels of carbon in the atmosphere originate from recently nucleosynthesized material that has been dredged up to the surface by deep convection during temporary shell burning events known as thermal pulses. Published spectral types for the star vary somewhat from C54 to C64, or N6 under an older system of classification.[2][13] The subscript 4 refers to the strength of the molecular carbon bands in the spectrum, an indicator of the relatively abundances of carbon in the atmosphere.
V Aquilae is a variable star of type SRb.[11] Its variability was first announced by George Knott in 1871.[15] It has a published period of 400 days, but other periods are found including 350 days and 2,270 days.[16]
References
- ^ a b Page Module:Citation/CS1/styles.css has no content.van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357. S2CID 18759600.Vizier catalog entry
- ^ a b c d Page Module:Citation/CS1/styles.css has no content.Samus, N. N.; Durlevich, O. V.; et al. (2009). "VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)". VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S. 1: B/GCVS. Bibcode:2009yCat....102025S.
- ^ Page Module:Citation/CS1/styles.css has no content.Jeste, Manali; Gong, Yan; Wong, Ka Tat; Menten, Karl M.; Kamiński, Tomasz; Wyrowski, Friedrich (2022). "Vibrationally excited HCN transitions in circumstellar envelopes of carbon-rich AGB stars". Astronomy and Astrophysics. 666: A69. arXiv:2206.12371. Bibcode:2022A&A...666A..69J. doi:10.1051/0004-6361/202243365.
- ^ Page Module:Citation/CS1/styles.css has no content.Nicolet, B. (October 1978). "Catalogue of homogeneous data in the UBV photoelectric photometric system". Astronomy & Astrophysics Supplement Series. 34: 1–49. Bibcode:1978A&AS...34....1N.
- ^ Page Module:Citation/CS1/styles.css has no content.Wilson, Ralph Elmer (1953). "General Catalogue of Stellar Radial Velocities". Carnegie Institute Washington D.C. Publication: 0. Bibcode:1953GCRV..C......0W.
- ^ a b c Template:Cite DR2
- ^ Page Module:Citation/CS1/styles.css has no content.Guandalini, R; Cristallo, S (2013). "Luminosities of carbon-rich asymptotic giant branch stars in the Milky Way". Astronomy & Astrophysics. 555: A120. arXiv:1305.4203. Bibcode:2013A&A...555A.120G. doi:10.1051/0004-6361/201321225. S2CID 54918450.
- ^ Page Module:Citation/CS1/styles.css has no content.Anders, F.; Khalatyan, A.; Chiappini, C.; Queiroz, A. B.; Santiago, B. X.; Jordi, C.; Girardi, L.; Brown, A. G. A.; Matijevič, G.; Monari, G.; Cantat-Gaudin, T.; Weiler, M.; Khan, S.; Miglio, A.; Carrillo, I.; Romero-Gómez, M.; Minchev, I.; De Jong, R. S.; Antoja, T.; Ramos, P.; Steinmetz, M.; Enke, H. (2019). "Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia DR2 stars brighter than G = 18". Astronomy and Astrophysics. 628: A94. arXiv:1904.11302. Bibcode:2019A&A...628A..94A. doi:10.1051/0004-6361/201935765. S2CID 131780028.
- ^ a b Page Module:Citation/CS1/styles.css has no content.McDonald, I.; Zijlstra, A. A.; Watson, R. A. (2017). "Fundamental parameters and infrared excesses of Tycho-Gaia stars". Monthly Notices of the Royal Astronomical Society. 471 (1): 770. arXiv:1706.02208. Bibcode:2017MNRAS.471..770M. doi:10.1093/mnras/stx1433. S2CID 73594365.
- ^ a b Page Module:Citation/CS1/styles.css has no content.Schöier, F. L; Ramstedt, S; Olofsson, H; Lindqvist, M; Bieging, J. H; Marvel, K. B (2013). "The abundance of HCN in circumstellar envelopes of AGB stars of different chemical type". Astronomy & Astrophysics. 550: A78. arXiv:1301.2129. Bibcode:2013A&A...550A..78S. doi:10.1051/0004-6361/201220400. S2CID 96447896.
- ^ a b Page Module:Citation/CS1/styles.css has no content.Lambert, David L.; Gustafsson, Bengt; Eriksson, Kjell; Hinkle, Kenneth H. (October 1986). "The chemical composition of carbon stars. I - Carbon, nitrogen, and oxygen in 30 cool carbon stars in the Galactic disk". Astrophysical Journal Supplement Series. 62: 373–425. Bibcode:1986ApJS...62..373L. doi:10.1086/191145.
- ^ Page Module:Citation/CS1/styles.css has no content."V* V Aql -- Semi-regular pulsating Star". SIMBAD. Centre de Données astronomiques de Strasbourg. Retrieved 2010-10-06.
- ^ Page Module:Citation/CS1/styles.css has no content.Skiff, B. A. (2014). "VizieR Online Data Catalog: Catalogue of Stellar Spectral Classifications (Skiff, 2009-2016)". VizieR On-line Data Catalog: B/Mk. Originally Published in: Lowell Observatory (October 2014). 1: B/mk. Bibcode:2014yCat....1.2023S.
- ^ Page Module:Citation/CS1/styles.css has no content."Hipparcos Tools Interactive Data Access". Hipparcos. ESA. Retrieved 8 December 2021.
- ^ Page Module:Citation/CS1/styles.css has no content.Cannon, Annie J. (1907). "Second catalogue of variable stars". Annals of Harvard College Observatory. 55: 1–94. Bibcode:1907AnHar..55....1C. Retrieved 21 November 2024.
- ^ Page Module:Citation/CS1/styles.css has no content.Olivier, E. A; Wood, P. R (2003). "On the Origin of Long Secondary Periods in Semiregular Variables". The Astrophysical Journal. 584 (2): 1035–1041. Bibcode:2003ApJ...584.1035O. doi:10.1086/345715.