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Discovery of a widely separated binary system of very low mass stars
- Source :
- Astronomy and Astrophysics-A&A, Astronomy and Astrophysics-A&A, EDP Sciences, 2005, 439, pp.L19. ⟨10.1051/0004-6361:200500149⟩, Astronomy and Astrophysics-A&A, EDP Sciences, 2005, 439, pp.L19-L22. ⟨10.1051/0004-6361:200500149⟩
- Publication Year :
- 2005
- Publisher :
- HAL CCSD, 2005.
-
Abstract
- We report our discovery of a nearby wide binary system, LP 714-37 AB. Phan-Bao et al. identified LP 714-37 as a mid-M dwarf during a cross-identification of the NLTT and DENIS catalogues. Our CCD images resolve the system into a binary with a projected angular separation of 1.8 arcsec, or 33 AU, and low-resolution optical spectra give spectral types of M5.5 (LP 714-37A) and M7.5 (LP 714-37B). This makes LP 714-37 AB one of very few widely separated (separation > 30 AU) very low-mass binary systems known in the field, and we discuss it in the context of the multiplicity properties of very low-mass stars and brown dwarfs.<br />Accepted by A&A Letters
- Subjects :
- Brown dwarf
FOS: Physical sciences
Binary number
Astrophysics
Stellar classification
01 natural sciences
binary stars
[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]
0103 physical sciences
Binary star
Binary system
010303 astronomy & astrophysics
Physics
individual star: DENIS-P J0410-1251
[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]
010308 nuclear & particles physics
Angular distance
Astrophysics (astro-ph)
Astronomy and Astrophysics
very low mass stars
Stars
individual star: LP 714-37
Space and Planetary Science
Low Mass
brown dwarfs
Subjects
Details
- Language :
- English
- ISSN :
- 00046361
- Database :
- OpenAIRE
- Journal :
- Astronomy and Astrophysics-A&A, Astronomy and Astrophysics-A&A, EDP Sciences, 2005, 439, pp.L19. ⟨10.1051/0004-6361:200500149⟩, Astronomy and Astrophysics-A&A, EDP Sciences, 2005, 439, pp.L19-L22. ⟨10.1051/0004-6361:200500149⟩
- Accession number :
- edsair.doi.dedup.....90f16e661434deaf8ffccfe52f23525c
- Full Text :
- https://doi.org/10.1051/0004-6361:200500149⟩