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BD Camelopardalis

From Wikipedia, the free encyclopedia
Star in the constellation Camelopardalis
BD Camelopardalis

Alight curve for BD Camelopardalis from Hipparcos data, adapted from Adelman (1998)[1]
Observation data
Epoch J2000      Equinox J2000
ConstellationCamelopardalis
Right ascension03h 42m 09.32551s[2]
Declination+63° 13′ 00.4686″[2]
Apparent magnitude (V)5.11[3]
Characteristics
Evolutionary stageAGB[4]
Spectral typeS3.5/2[5] (M4III)[6]
U−Bcolor index1.82[7]
B−Vcolor index1.63[7]
R−Icolor index1.39
Variable typeLb[8]
Astrometry
Radial velocity (Rv)−22.28[9] km/s
Proper motion (μ)RA: −17.877mas/yr[2]
Dec.: +20.052mas/yr[2]
Parallax (π)4.2671±0.2581 mas[2]
Distance750+36
−49
 ly
(231+11
−15
 pc)[10]
Absolute magnitude (MV)−0.90
Orbit[11]
PrimaryBD Cam A
CompanionBD Cam B
Period (P)596.2 days
Eccentricity (e)0.088
Inclination (i)105.6°
Longitude of the node (Ω)162.1°
Periastronepoch (T)2442794.5
Argument of periastron (ω)
(secondary)
334.3°
Details
Red giant primary
Mass2.68[12] M
Radius148+8
−10
[13] R
Luminosity2,000[14] L
Surface gravity (log g)1.5[12] cgs
Temperature3,600±150[14] K
Metallicity−0.25[12]
Other designations
BD Cam,SAO 12874,BD+62°597,HD 22649,HIP 17296,FK5 129,HR 1105[15]
Database references
SIMBADdata

BD Camelopardalis is anS star andsymbiotic star in the constellationCamelopardalis. It is a 5thmagnitude star, and is visible to thenaked eye under good observing conditions. It was recognized as aspectroscopic binary star in 1922, and its orbital solution published in 1984;[16] it has a 596-day orbital period. A spectroscopic composition analysis was done of the red giant primary star in 1986.[17]

Description

[edit]

Although the star's spectrum shows the spectral features of zirconium oxide which definespectral class S, BD Cam shows notechnetium lines in its spectrum. It is believed to be an "extrinsic" S star, one whoses-process element excesses originate in a binary companion star.

In 1928,Joel Stebbins andCharles Morse Huffer announced that the star, then called HR 1105, is avariable star, based on observations made atWashburn Observatory.[18] It was given itsvariable star designation, BD Camelopardalis, in 1977.[19] The system displays only minimal variations in thevisible, but the presence of the companion and its interactions with thestellar wind of the visiblered giant makes for easily observed time-variable spectral features in theultraviolet and in thenear infrared spectral line ofhelium.

At times BD Cam is the brightest S star in the visible sky, because other bright S stars areMira variables or other types of variable star with large changes in apparent brightness. Its own brightness variability in the visible part of the spectrum is modest.

On the basis of the measurement of radial velocities of the line components it is concluded that the helium emission originates in the vicinity of the inner Lagrangian point of the system, indicating a gas motion from the red giant primary, directed to the secondary, with a velocity of about 5 km/s. At the same time, there is a high-velocity, hot wind outwards from the primary red giant with a velocity of about 50 km/s.

— Shcherbakov, A. G. and Tuominen, I.

However, HR 1105 appears to have a highly variable UV companion. In 1982, no UV flux was discerned for this system, but by 1986 C IV was strong, increasing by a factor of 3 in 1987 with prominent lines of Si III, C III, O III, Si IV, and N V.

— Ake, Thomas B., III; Johnson, Hollis R. and Perry, Benjamin F., Jr.

References

[edit]
  1. ^Adelman, S. J. (May 1998). "BVRI photometry of the extrinsic S star HR 1105".Astronomy & Astrophysics.333:952–955.Bibcode:1998A&A...333..952A.
  2. ^abcdVallenari, 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 atVizieR.
  3. ^Ducati, J. R. (2002). "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system".CDS/ADC Collection of Electronic Catalogues.2237.Bibcode:2002yCat.2237....0D.
  4. ^Guandalini, R.; Busso, M. (2008). "Infrared photometry and evolution of mass-losing AGB stars".Astronomy and Astrophysics.488 (2):675–684.arXiv:0806.4591.Bibcode:2008A&A...488..675G.doi:10.1051/0004-6361:200809932.S2CID 14294870.
  5. ^Keenan, P. C.; Boeshaar, P. C. (1980)."Spectral types of S and SC stars on the revised MK system".The Astrophysical Journal Supplement Series.43: 379.Bibcode:1980ApJS...43..379K.doi:10.1086/190673.
  6. ^Yamashita, Y. (1967). "MK Spectral Types of Bright M-Type Stars".Publications of the Dominion Astrophysical Observatory Victoria.13: 47.Bibcode:1967PDAO...13...47Y.
  7. ^abvan Leeuwen, F. (1970)."Photometry of high-luminosity M-type stars".Astrophysical Journal.162: 217.Bibcode:1970ApJ...162..217L.doi:10.1086/150648.
  8. ^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.Bibcode:2009yCat....102025S.
  9. ^Pourbaix, D.; et al. (2004). "SB9: The ninth catalogue of spectroscopic binary orbits".Astronomy and Astrophysics.424 (2):727–732.arXiv:astro-ph/0406573.Bibcode:2004A&A...424..727P.doi:10.1051/0004-6361:20041213.
  10. ^Bailer-Jones, C. A. L.; Rybizki, J.; Fouesneau, M.; Demleitner, M.; Andrae, R. (2021-03-01)."Estimating distances from parallaxes. V: Geometric and photogeometric distances to 1.47 billion stars in Gaia Early Data Release 3".The Astronomical Journal.161 (3): 147.arXiv:2012.05220.Bibcode:2021AJ....161..147B.doi:10.3847/1538-3881/abd806.ISSN 0004-6256. Data about this star can be seenhere.
  11. ^Pourbaix, D. (2000). "Re-processing the Hipparcos Transit Data and Intermediate Astrometric Data of spectroscopic binaries. I. Ba, CH and Tc-poor S stars".Astronomy and Astrophysics Supplement.145:161–183.arXiv:astro-ph/0006175.Bibcode:2000A&AS..145..161P.doi:10.1051/aas:2000346.S2CID 15990458.
  12. ^abcKhalatyan, A.; Anders, F.; Chiappini, C.; Queiroz, A. B. A.; Nepal, S.; Dal Ponte, M.; Jordi, C.; Guiglion, G.; Valentini, M.; Torralba Elipe, G.; Steinmetz, M.; Pantaleoni-González, M.; Malhotra, S.; Jiménez-Arranz, Ó.; Enke, H.; Casamiquela, L.; Ardèvol, J. (2024). "Transferring spectroscopic stellar labels to 217 million Gaia DR3 XP stars with SHBoost".Astronomy and Astrophysics.691: A98.arXiv:2407.06963.Bibcode:2024A&A...691A..98K.doi:10.1051/0004-6361/202451427.
  13. ^Baines, Ellyn K.; Clark, James H.; Kingsley, Bradley I.; Schmitt, Henrique R.; Stone, Jordan M. (2025-05-07)."Vintage NPOI: New and Updated Angular Diameters for 145 Stars".The Astronomical Journal.169 (6): 293.arXiv:2506.02912.Bibcode:2025AJ....169..293B.doi:10.3847/1538-3881/adc930.ISSN 1538-3881.
  14. ^abCharbonnel, C.; Lagarde, N.; Jasniewicz, G.; North, P. L.; Shetrone, M.; Krugler Hollek, J.; Smith, V. V.; Smiljanic, R.; Palacios, A.; Ottoni, G. (2020-01-01). "Lithium in red giant stars: Constraining non-standard mixing with large surveys in the Gaia era".Astronomy and Astrophysics.633: A34.arXiv:1910.12732.Bibcode:2020A&A...633A..34C.doi:10.1051/0004-6361/201936360.ISSN 0004-6361.BD Cam's database entry atVizieR.
  15. ^"BD Cam".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved27 December 2016.
  16. ^Griffin, R.F. (1984). "Spectroscopic binary orbits from photoelectric radial velocities. Paper 58: HR 1105".Observatory.104:224–231.Bibcode:1984Obs...104..224G.
  17. ^Smith, V.V.; Lambert, D.L. (1986)."The chemical composition of red giants. II - Helium burning and the s-process in the MS and S stars".Astrophysical Journal.311:843–863.Bibcode:1986ApJ...311..843S.doi:10.1086/164823.
  18. ^Stebbins, Joel; Huffer, C. M. (1928)."The Constancy of the Light of Red Stars".Publications of the Washburn Observatory.15:137–174.Bibcode:1928PWasO..15..137S. Retrieved5 December 2024.
  19. ^Kukarkin, B. V.; Kholopov, P. N.; Fedorovich, V. P.; Kireyeva, N. N.; Kukarkina, N. P.; Medvedeva, G. I.; Perova, N. B. (March 1977)."62nd Name-List of Variable Stars"(PDF).Information Bulletin on Variable Stars.1248: 1.Bibcode:1977IBVS.1248....1K. Retrieved29 December 2024.

Further reading

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