The variability of Gliese 908 was confirmed in 1994, although no period could be detected in its brightness changes.[16] It was entered into the
General Catalogue of Variable Stars in 1997.[17]
Gliese 908 is a cool
main sequence star, a red dwarf, with a
spectral class of M1V Fe-1. The suffix indicates a noticeable deficiency in heavy elements.[4]
^
abcPerryman; et al. (1997).
"HIP 117473". The Hipparcos and Tycho Catalogues.
Archived from the original on 2016-03-04. Retrieved 2015-09-21.
^
abSamus, 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: B/gcvs.
Bibcode:
2009yCat....102025S.
^
abKeenan, Philip C.; McNeil, Raymond C. (1989). "The Perkins Catalog of Revised MK Types for the Cooler Stars". The Astrophysical Journal Supplement Series. 71: 245.
Bibcode:
1989ApJS...71..245K.
doi:
10.1086/191373.
^Gliese, W.; Jahreiß, H. (1991).
"Gl 908". Preliminary Version of the Third Catalogue of Nearby Stars.
Archived from the original on 2016-03-04. Retrieved 2015-09-21.
^Luyten, Willem Jacob (1979).
"LHS 550". LHS Catalogue, 2nd Edition.
Archived from the original on 2020-09-25. Retrieved 2015-10-15.
^Van Altena W. F.; Lee J. T.; Hoffleit E. D. (1995).
"GCTP 5763". The General Catalogue of Trigonometric Stellar Parallaxes (Fourth ed.).
Archived from the original on 2016-03-04. Retrieved 2015-09-21.
^Perryman; et al. (1997).
"HIP 117473". The Hipparcos and Tycho Catalogues.
Archived from the original on 2016-03-04. Retrieved 2015-09-21.
^Kazarovets, E. V.; Samus, N. N. (1997). "The 73rd Name-List of Variable Stars". Information Bulletin on Variable Stars. 4471: 1.
Bibcode:
1997IBVS.4471....1K.
The variability of Gliese 908 was confirmed in 1994, although no period could be detected in its brightness changes.[16] It was entered into the
General Catalogue of Variable Stars in 1997.[17]
Gliese 908 is a cool
main sequence star, a red dwarf, with a
spectral class of M1V Fe-1. The suffix indicates a noticeable deficiency in heavy elements.[4]
^
abcPerryman; et al. (1997).
"HIP 117473". The Hipparcos and Tycho Catalogues.
Archived from the original on 2016-03-04. Retrieved 2015-09-21.
^
abSamus, 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: B/gcvs.
Bibcode:
2009yCat....102025S.
^
abKeenan, Philip C.; McNeil, Raymond C. (1989). "The Perkins Catalog of Revised MK Types for the Cooler Stars". The Astrophysical Journal Supplement Series. 71: 245.
Bibcode:
1989ApJS...71..245K.
doi:
10.1086/191373.
^Gliese, W.; Jahreiß, H. (1991).
"Gl 908". Preliminary Version of the Third Catalogue of Nearby Stars.
Archived from the original on 2016-03-04. Retrieved 2015-09-21.
^Luyten, Willem Jacob (1979).
"LHS 550". LHS Catalogue, 2nd Edition.
Archived from the original on 2020-09-25. Retrieved 2015-10-15.
^Van Altena W. F.; Lee J. T.; Hoffleit E. D. (1995).
"GCTP 5763". The General Catalogue of Trigonometric Stellar Parallaxes (Fourth ed.).
Archived from the original on 2016-03-04. Retrieved 2015-09-21.
^Perryman; et al. (1997).
"HIP 117473". The Hipparcos and Tycho Catalogues.
Archived from the original on 2016-03-04. Retrieved 2015-09-21.
^Kazarovets, E. V.; Samus, N. N. (1997). "The 73rd Name-List of Variable Stars". Information Bulletin on Variable Stars. 4471: 1.
Bibcode:
1997IBVS.4471....1K.