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White drawf star in the northern constellation of Hercules
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,
[2] it is too faint to be visible to the naked eye. Its
trigonometric parallax from the
Gaia mission is 62.9
″ ,
[1] 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.
[3] 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.
[7] Ross 640 has a spectrum characterized by hydrogen
Balmer lines in the visible and very strong ionized magnesium lines in the ultraviolet.
[9] The presence of heavy elements in the photosphere of Ross 640 indicates that it recently
accreted rocky debris from its planetary system.
References
^
a
b
c
d
e 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 .
^
a
b Bergeron, P.; Leggett, S. K.; Ruiz, María Teresa (2001). "Photometric and Spectroscopic Analysis of Cool White Dwarfs with Trigonometric Parallax Measurements". The Astrophysical Journal Supplement Series . 133 (2): 413–450.
arXiv :
astro-ph/0011286 .
Bibcode :
2001ApJS..133..413B .
doi :
10.1086/320356 .
ISSN
0067-0049 .
S2CID
15511301 .
^
a
b Wesemael, F.; et al. (1993).
"An atlas of optical spectra of white-dwarf stars" . Publications of the Astronomical Society of the Pacific . 105 : 761.
Bibcode :
1993PASP..105..761W .
doi :
10.1086/133228 .
S2CID
122605705 .
^ 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.
arXiv :
1505.02297 .
Bibcode :
2015ApJS..219...19L .
doi :
10.1088/0067-0049/219/2/19 .
S2CID
118494290 .
^
a
b Toonen, S.; Hollands, M.; Gänsicke, B. T.; Boekholt, T. (2017). "The binarity of the local white dwarf population". Astronomy and Astrophysics . 602 : A16.
arXiv :
1703.06893 .
Bibcode :
2017A&A...602A..16T .
doi :
10.1051/0004-6361/201629978 .
S2CID
12367523 .
^
a
b 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.
arXiv :
1606.01236 .
Bibcode :
2016MNRAS.462.2295H .
doi :
10.1093/mnras/stw1357 .
hdl :
10150/621732 .
^
a
b 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.
arXiv :
1807.06616 .
Bibcode :
2018ApJ...863..184B .
doi :
10.3847/1538-4357/aad4a9 .
S2CID
119347098 .
^
"ross 640" .
SIMBAD .
Centre de données astronomiques de Strasbourg . Retrieved 2019-08-20 .
^ 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 .