HR 1884
Binary star system in the constellation Auriga
HR 1884 is a spectroscopic binary star in the constellation Auriga . The primary is a G type supergiant star while the secondary is probably a B type main sequence star.
The possible spectroscopic binary nature of the star was first noted in 1983 by Gilbert Burki and Michel Mayor in a paper on the rate of binaries among supergiant stars. In the same year, William P. Bidelman noted that the stellar spectrum was composite indicating a companion star. Confirmation of spectroscopic binary status and a preliminary orbit was published in 1998 by R. Paul Butler , a much more accurate orbit was published in 2015 by Roger Griffin.
References
↑ Roman, Nancy G. (1987). "Identification of a constellation from a position" . Publications of the Astronomical Society of the Pacific . 99 (617): 695. Bibcode :1987PASP...99..695R . doi :10.1086/132034 .
Constellation record for this object at VizieR .
1 2 3 4 5 6 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 .
1 2 3 Argue, A. N. (1966). "UBV photometry of 550 F, G and K type stars" . Monthly Notices of the Royal Astronomical Society . 133 (4): 175– 493. Bibcode :1966MNRAS.133..475A . doi :10.1093/mnras/133.4.475 .
↑ Bidelman, William P. (1957). "Spectral Classification of Stars Noted on Case Objective-Prism Plates. I" . Publications of the Astronomical Society of the Pacific . 69 (407): 147– 152. Bibcode :1957PASP...69..147B . doi :10.1086/127034 .
1 2 3 4 5 Griffin, R. F. (2015). "Spectroscopic binary orbits from photoelectric radial velocities. Paper 241: HR 1884, HD 174103, HD 182563, and HR 8442, with a note on zeta Cephei". The Observatory . 135 : 71– 95. Bibcode :2015Obs...135...71G .
↑ Kovtyukh, V. V.; Chekhonadskikh, F. A.; Luck, R. E.; Soubiran, C.; Yasinskaya, M. P.; Belik, S. I. (2010). "Accurate luminosities for F-G supergiants from FeII/FeI line depth ratios" . Monthly Notices of the Royal Astronomical Society . 408 (3): 1568. Bibcode :2010MNRAS.408.1568K . doi :10.1111/j.1365-2966.2010.17217.x .
1 2 3 Brown, 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 . Gaia DR2 record for this source at VizieR .
1 2 Luck, R. Earle (2014). "Parameters and Abundances in Luminous Stars" . The Astronomical Journal . 147 (6): 137. Bibcode :2014AJ....147..137L . doi :10.1088/0004-6256/147/6/137 .
↑ De Medeiros, J. R.; Udry, S.; Burki, G.; Mayor, M. (2002). "A catalog of rotational and radial velocities for evolved stars. II. Ib supergiant stars" . Astronomy and Astrophysics . 395 : 97– 98. Bibcode :2002A& A...395...97D . doi :10.1051/0004-6361:20021214 .
↑ Burki, G.; Mayor, M. (1983). "Nineteen new spectroscopic binaries and the rate of binary stars among F-M supergiants". Astronomy and Astrophysics . 124 (2): 256– 266. Bibcode :1983A& A...124..256B .
↑ Bidelman, W. P. (1983). "Objective-prism discoveries in the northern sky. I". Astronomical Journal . 88 : 1182– 1186. Bibcode :1983AJ.....88.1182B . doi :10.1086/113408 .
↑ Butler, R. Paul (1998). "A Precision Velocity Study of Photometrically Stable Stars in the Cepheid Instability Strip". Astrophysical Journal . 494 (1): 342– 365. Bibcode :1998ApJ...494..342B . CiteSeerX 10.1.1.37.7095 . doi :10.1086/305195 . S2CID 119678211 .