Astronomy:Ross 640

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Short description: White dwarf star in the northern constellation of Hercules

Coordinates: Sky map 16h 28m 25.00s, +36° 46′ 15.9″

Ross 640
Observation data
Equinox J2000.0]] (ICRS)
Constellation Hercules[1]
Right ascension  16h 28m 25.0031s[2]
Declination +36° 46′ 15.847″[2]
Apparent magnitude (V) 13.83[3]
Characteristics
Evolutionary stage white dwarf
Spectral type DZA5.5[4]
Astrometry
Proper motion (μ) RA: −494.230(15)[2] mas/yr
Dec.: 746.698(18)[2] mas/yr
Parallax (π)62.9109 ± 0.0143[2] mas
Distance51.84 ± 0.01 ly
(15.895 ± 0.004 pc)
Absolute magnitude (MV)+13.01[5]
Details
Mass0.58±0.03[6] M☉
Luminosity0.0007[6] L☉
Surface gravity (log g)7.76[7] cgs
Temperature8,100[8] K
Age1.02[7] Gyr
Other designations
GJ 626.2, LTT 14906, WD 1626+368[9]
Database references
SIMBADdata

Ross 640 is a white dwarf star in the northern constellation of Hercules, positioned near the constellation border with Corona Borealis. With an apparent visual magnitude of 13.83,[3] it is too faint to be visible to the naked eye. Its trigonometric parallax from the Gaia mission is 62.9″,[2] corresponding to a distance of 52 light-years (15.9 parsecs).

This compact star has a stellar classification of DZA5.5, indicating a metal-rich atmosphere accompanied by weaker lines of hydrogen.[4] A detailed analysis of its spectrum revealed that Ross 640 is a relatively cool white dwarf with an effective temperature of approximately 8,100 K, which means that it has been in the white dwarf phase for slightly more than 1 billion years.[8] Ross 640 has a spectrum characterized by hydrogen Balmer lines in the visible and very strong ionized magnesium lines in the ultraviolet.[10] The presence of heavy elements in the photosphere of Ross 640 indicates that it recently accreted rocky debris from its planetary system.

References

  1. ↑ Roman, Nancy G. (1987). "Identification of a constellation from a position". Publications of the Astronomical Society of the Pacific 99 (617): 695. doi:10.1086/132034. Bibcode: 1987PASP...99..695R  Constellation record for this object at VizieR.
  2. ↑ 2.0 2.1 2.2 2.3 2.4 Vallenari, A. et al. (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics. doi:10.1051/0004-6361/202243940  Gaia DR3 record for this source at VizieR.
  3. ↑ 3.0 3.1 Bergeron, P.; Leggett, S. K.; Ruiz, María Teresa (2001). "Photometric and Spectroscopic Analysis of Cool White Dwarfs with Trigonometric Parallax Measurements" (in en). The Astrophysical Journal Supplement Series 133 (2): 413–450. doi:10.1086/320356. ISSN 0067-0049. Bibcode: 2001ApJS..133..413B. 
  4. ↑ 4.0 4.1 Wesemael, F. et al. (1993). "An atlas of optical spectra of white-dwarf stars". Publications of the Astronomical Society of the Pacific 105: 761. doi:10.1086/133228. Bibcode: 1993PASP..105..761W. 
  5. ↑ Limoges, M. -M; Bergeron, P.; Lépine, S. (2015). "Physical Properties of the Current Census of Northern White Dwarfs within 40 pc of the Sun". The Astrophysical Journal Supplement Series 219 (2): 19. doi:10.1088/0067-0049/219/2/19. Bibcode: 2015ApJS..219...19L. 
  6. ↑ 6.0 6.1 Toonen, S.; Hollands, M.; Gänsicke, B. T.; Boekholt, T. (2017). "The binarity of the local white dwarf population". Astronomy and Astrophysics 602: A16. doi:10.1051/0004-6361/201629978. Bibcode: 2017A&A...602A..16T. 
  7. ↑ 7.0 7.1 Holberg, J. B.; Oswalt, T. D.; Sion, E. M.; McCook, G. P. (2016). "The 25 parsec local white dwarf population". Monthly Notices of the Royal Astronomical Society 462 (3): 2295. doi:10.1093/mnras/stw1357. Bibcode: 2016MNRAS.462.2295H. 
  8. ↑ 8.0 8.1 Blouin, S.; Dufour, P.; Allard, N. F. (23 August 2018). "A New Generation of Cool White Dwarf Atmosphere Models. I. Theoretical Framework and Applications to DZ Stars". The Astrophysical Journal 863 (2): 184. doi:10.3847/1538-4357/aad4a9. Bibcode: 2018ApJ...863..184B. 
  9. ↑ "ross 640". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=ross+640. 
  10. ↑ Zeidler-K.T., E.-M.; Weidemann, V.; Koester, D. (1986). "Metal abundances in helium-rich white dwarf atmospheres". Astronomy & Astrophysics 155 (2): 356–370. Bibcode: 1986A&A...155..356Z.