| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Virgo |
| Right ascension | 13h 58m 24.860s [2] |
| Declination | −01° 39′ 38.95″ [2] |
| Apparent magnitude (V) | 9.60 - 10.56 [3] |
| Characteristics | |
| Evolutionary stage | Main sequence |
| Spectral type | G0 V + G2 V [4] |
| B−V color index | 0.650±0.043 [5] |
| Variable type | Algol + RS CVn [3] |
| Astrometry | |
| Radial velocity (Rv) | −22.80±2.7 [6] km/s |
| Proper motion (μ) |
RA: 2.672
mas/
yr
[2] Dec.: −5.742 mas/ yr [2] |
| Parallax (π) | 6.6834 ± 0.0181 mas [2] |
| Distance | 488 ± 1
ly (149.6 ± 0.4 pc) |
| Orbit [4] | |
| Period (P) | 0.8169 d |
| Semi-major axis (a) | ≥1.55 Gm (2.23 R☉) |
| Eccentricity (e) | 0.0 |
| Inclination (i) | 87.5±0.8 [7]° |
| Periastron epoch (T) | 2,431,241.389±1.0 JD |
|
Argument of periastron (ω) (secondary) | 0.0° |
|
Semi-amplitude (K1) (primary) | 137.8 km/s |
| Semi-amplitude (K2) (secondary) | 135.2 km/s |
| Details | |
| Component 1 | |
| Mass | 1.173±0.006 [7] M☉ |
| Radius | 1.22±0.05 [7] R☉ |
| Luminosity | 2.19 [8] L☉ |
| Surface gravity (log g) | 4.30 [8] cgs |
| Temperature | 5,969±11 [9] K |
| Metallicity [Fe/H] | +0.1 [8] dex |
| Component 2 | |
| Mass | 1.046±0.005 [7] M☉ |
| Radius | 1.11±0.04 [7] R☉ |
| Luminosity | 1.20 [8] L☉ |
| Surface gravity (log g) | 4.35 [8] cgs |
| Temperature | 5,500 [9] K |
| Metallicity [Fe/H] | −0.3 [8] dex |
| Other designations | |
| Database references | |
| SIMBAD | data |
BH Virginis is a binary star system in the equatorial constellation of Virgo. With a typical apparent visual magnitude of 9.6, [3] it is too faint to be visible to the naked eye. Based on parallax measurements, it is located at a distance of approximately 488 light years from the Sun. [2] The system is drifting closer with a net radial velocity of −23 km/s. [6]
This system was determined to be a short period variable star by C. Hoffmeister in 1935. [11] W. Zessewitsch found a period of 19.6 hours for the system in 1944. In 1957, M. Kitamura and associates refined the light curve of this Algol-type eclipsing variable and discovered some irregular fluctuations not explained by the eclipse cycle. [12] R. H. Koch in 1967 reported observing a change in the depth of the primary eclipse. [13] In 1982, M. Hoffmann concluded that both stars are intrinsically variable, indicating this is an RS Canum Venaticorum variable system. [14]
This is a near-contact [15] binary system with a circular orbit having a period of 19.61 hours. [4] The orbital plane is inclined at an angle of 88° to the line of sight from the Earth, [7] allowing both components to eclipse each other once per orbit. During the deep [4] primary eclipse the system decreases in brightness by 0.96 magnitude, while the shallower secondary eclipse decreases the system by 0.64 magnitude. [15] Cyclical oscillations in the orbital period have been observed with two short-term periods of 9.2 and 11.8 years, and a longer-term oscillation of 51.7 years. The short term oscillations may be due to magnetic activity on the stars, while the longer period could be caused by an unseen third body. [16]
Both components of this system are G-type main-sequence stars, with stellar classifications of G0V and G2V, respectively. [4] Evidence of star spots have been found on both stars, but appear to be predominantly on the secondary component. [9] The two stars are somewhat larger and more massive than the Sun. [7]
References
- ^ MAST: Barbara A. Mikulski Archive for Space Telescopes, Space Telescope Science Institute, retrieved 8 December 2021.
- ^ a b c d e Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics. 649: A1. arXiv: 2012.01533. Bibcode: 2021A&A...649A...1G. doi: 10.1051/0004-6361/202039657. S2CID 227254300. (Erratum: doi: 10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
- ^ a b c Samus, N. N.; et al. (2017), "General Catalogue of Variable Stars", Astronomy Reports, 5.1, 61 (1): 80–88, Bibcode: 2017ARep...61...80S, doi: 10.1134/S1063772917010085, S2CID 125853869.
- ^ a b c d e Abt, Helmut A. (October 1965), "Spectrographic Measures of the Eclipsing System BH Virginis", Publications of the Astronomical Society of the Pacific, 77 (458): 367, Bibcode: 1965PASP...77..367A, doi: 10.1086/128233, S2CID 121053195.
- ^ Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters, 38 (5): 331–346, arXiv: 1108.4971, Bibcode: 2012AstL...38..331A, doi: 10.1134/S1063773712050015, S2CID 119257644.
- ^ a b Karataș, Yüksel; et al. (2004), "Kinematics of chromospherically active binaries and evidence of an orbital period decrease in binary evolution", Monthly Notices of the Royal Astronomical Society, 349 (3): 1069–1092, arXiv: astro-ph/0404219, Bibcode: 2004MNRAS.349.1069K, doi: 10.1111/j.1365-2966.2004.07588.x, S2CID 15290475.
- ^ a b c d e f g Kjurkchieva, D. P.; et al. (September 2004), "Spectroscopic and photometric observations of the short-period RS CVn-type star BH Virginis", Astronomy and Astrophysics, 424 (3): 993–1002, Bibcode: 2004A&A...424..993K, doi: 10.1051/0004-6361:20035902.
- ^ a b c d e f Clement, R.; et al. (September 1997), "Absolute parameters for binary systems. I. The active binary BH Virginis", Astronomy and Astrophysics Supplement Series, 124 (3): 499–508, Bibcode: 1997A&AS..124..499C, doi: 10.1051/aas:1997367.
- ^ a b c Xiang, Fuyuan; et al. (October 2007), "Evidence of Hot Spot Activity on BH Virginis", Publications of the Astronomical Society of Japan, 59 (5): 955–960, Bibcode: 2007PASJ...59..955X, doi: 10.1093/pasj/59.5.955.
- ^ "BH Vir", SIMBAD, Centre de données astronomiques de Strasbourg, retrieved 2022-06-10.
- ^ Hoffmeister, Cuno (June 1935), "162 neue Veräderliche", Astronomische Nachrichten, 255 (22): 401, Bibcode: 1935AN....255..401H, doi: 10.1002/asna.19352552202. Listed as "– 0 2769" then "HD 121909" in a footnote.
- ^ Kitamura, M.; et al. (1957), "A Photoelectric Study of the Eclipsing System BH Virginis", Publications of the Astronomical Society of Japan, 9: 191, Bibcode: 1957PASJ....9..191K.
- ^ Koch, Robert H. (April 1967), "The complicated eclipsing binary, BH Virginis", Astronomical Journal, 72: 411, Bibcode: 1967AJ.....72..411K, doi: 10.1086/110243.
- ^ Hoffmann, M. (March 1982), "The variable light curve of BH Vir", Astronomy and Astrophysics Supplement Series, 47: 561–568, Bibcode: 1982A&AS...47..561H.
- ^ a b Avvakumova, E. A.; et al. (October 2013), "Eclipsing variables: Catalogue and classification", Astronomische Nachrichten, 334 (8): 860, Bibcode: 2013AN....334..860A, doi: 10.1002/asna.201311942, hdl: 10995/27061.
- ^ Tian, Yong-Po; et al. (June 2008), "On the Period Variations of BH Virginis", Publications of the Astronomical Society of Japan, 60 (3): 571–575, Bibcode: 2008PASJ...60..571T, doi: 10.1093/pasj/60.3.571.
Further reading
- Kozhevnikova, A. V.; et al. (November 2007), "Long-term starspot activity of the eclipsing binaries BH Vir and WY Cnc", Astronomy Reports, 51 (11): 932–946, Bibcode: 2007ARep...51..932K, doi: 10.1134/S1063772907110066, S2CID 120895929.
- Xiang, Fu Yuan; Zhou, Yi Chun (June 2004), "A Photometric Analysis and Spot Activity of BH Virginis", Publications of the Astronomical Society of Japan, 56 (3): 469–474, Bibcode: 2004PASJ...56..469X, doi: 10.1093/pasj/56.3.469.
- Xiang, F. Y.; Zhou, Y. C. (January 2004), "The spot activity of BH Virginis", New Astronomy, 9 (1): 27–31, Bibcode: 2004NewA....9...27X, doi: 10.1016/j.newast.2003.07.001.
- Arevalo, M. J.; et al. (January 2002), "J and K Infrared Light Curves of the Active Binary BH Vir", Information Bulletin on Variable Stars, 5222: 1, Bibcode: 2002IBVS.5222....1A.
- Xiang, F. Y.; et al. (October 2000), "Star-spots activity on BH Virginis", Astronomy and Astrophysics Supplement Series, 146: 7–12, Bibcode: 2000A&AS..146....7X, doi: 10.1051/aas:2000260.
- Qian, Shengbang; et al. (2000), "Orbital Period Studies of RS CVn-type binaries III. BH Virginis", Astrophysics and Space Science, 274 (4): 859–866, Bibcode: 2000Ap&SS.274..859Q, doi: 10.1023/A:1026512806446, S2CID 189838086.
- Popper, Daniel M. (September 1997), "Orbits of detached main-sequence eclipsing binaries of types late F to K. II. UV leonis, UV piscium, and BH virginis", The Astronomical Journal, 114: 1195, Bibcode: 1997AJ....114.1195P, doi: 10.1086/118552.
- Xiang, F. Y.; Liu, Q. Y. (August 1997), "The variable light curve of BH Virginis", Astronomy and Astrophysics Supplement Series, 124 (2): 281–282, Bibcode: 1997A&AS..124..281X, doi: 10.1051/aas:1997191.
- Lazaro, C.; Arevalo, M. J. (June 1997), "Time-Resolved Spectroscopy of RS CVn Short-Period Systems. I. CG CYG, BH VIR, and ER VUL", Astronomical Journal, 113: 2283, Bibcode: 1997AJ....113.2283L, doi: 10.1086/118439.
- Clement, R.; et al. (May 1997), "Four colour photometry of late-type binary systems. II. New light curves of BH Virginis", Astronomy and Astrophysics Supplement Series, 123: 59–61, Bibcode: 1997A&AS..123...59C, doi: 10.1051/aas:1997343.
- Heckert, P. A.; Summers, D. L. (August 1995), "1994 photometry of BH Virginis", Information Bulletin on Variable Stars, 4225: 1, Bibcode: 1995IBVS.4225....1H.
- Heckert, P. A.; Summers, D. L. (August 1994), "1993 BVRI Photometry of BH Virginis", Information Bulletin on Variable Stars, 4062: 1, Bibcode: 1994IBVS.4062....1H.
- Zhai, D. S.; et al. (October 1990), "An analysis of basic parameters and SPOT activities of the solar-type binary system BH Virginis", Astronomy and Astrophysics, 237: 148, Bibcode: 1990A&A...237..148Z.
- Arévalo, M. J.; Lázaro, C. (July 1990), "The Photometric Behaviour of BH Vir", Astrophysics and Space Science, 169 (1–2): 245–246, Bibcode: 1990Ap&SS.169..245A, doi: 10.1007/BF00640724, S2CID 124271181.
- Derman, E.; et al. (December 1989), "1989 Light Curves of BH Vir", Information Bulletin on Variable Stars, 3404: 1, Bibcode: 1989IBVS.3404....1D.
- Zeilik, M.; et al. (May 1990), "Long-Term Starspot Activity of Short-Period RS Canum Venaticorum Stars. III. BH Virginis", Astrophysical Journal, 354: 352, Bibcode: 1990ApJ...354..352Z, doi: 10.1086/168693.
- Arevalo, M. J.; et al. (December 1987), "1986 BV Light Curves of BH Virginis", Information Bulletin on Variable Stars, 3117: 1, Bibcode: 1987IBVS.3117....1A.
- Scaltriti, F.; et al. (August 1985), "Photometry of southern stars. II. Further evidence of spots in the eclipsing binary BH Virginis", Astronomy and Astrophysics, 149: 11–14, Bibcode: 1985A&A...149...11S.
- Giuricin, G.; et al. (January 1984), "Lightcurve analysis for the eclipsing binaries ST Car, RY Ind and BH Vir", Monthly Notices of the Royal Astronomical Society, 206 (2): 305–313, Bibcode: 1984MNRAS.206..305G, doi: 10.1093/mnras/206.2.305.
- Botsula, R. A. (1978), "Instability in detached binary systems of the main sequence with solar-type components. II. BH Virginis", Peremennye Zvezdy (in Russian), 20: 577–587, Bibcode: 1978PZ.....20..577B.
- Whitney, B. S. (1955), "Minima and periods of eclipsing stars", Astronomical Journal, 60: 453, Bibcode: 1955AJ.....60..453W, doi: 10.1086/107258.
