The binary system L151-81A/B : a potential test of accretion theory

M. A. Wood; T. D. Oswalt

doi:10.1086/186470

The binary system L151-81A/B : a potential test of accretion theory

M. A. Wood
, T. D. Oswalt

Research output: Contribution to journal › Article › peer-review

Original language	American English
Journal	The Astrophysical Journal
Volume	394
DOIs	https://doi.org/10.1086/186470
State	Published - Aug 1 1992

Disciplines

Astrophysics and Astronomy
Physics

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@article{f76ee0fe4b9c4797a8963f78f11884b7,

title = "The binary system L151-81A/B : a potential test of accretion theory",

author = "Wood, \{M. A.\} and Oswalt, \{T. D.\}",

note = "The common proper motion binary white dwarf system L151 - 81A/B, consisting of two (a DA and a DB) components is particularly interesting because the cooler (older) hydrogen-atmosphere (DA) star has T(eff) = 12,000 +/-2000 K, nominally placing it within the ZZ Ceti instability strip.",

year = "1992",

month = aug,

day = "1",

doi = "10.1086/186470",

language = "American English",

volume = "394",

journal = "The Astrophysical Journal",

issn = "1538-4357",

publisher = "Institute of Physics Publishing, Inc.",

}

TY - JOUR

T1 - The binary system L151-81A/B : a potential test of accretion theory

AU - Wood, M. A.

AU - Oswalt, T. D.

N1 - The common proper motion binary white dwarf system L151 - 81A/B, consisting of two (a DA and a DB) components is particularly interesting because the cooler (older) hydrogen-atmosphere (DA) star has T(eff) = 12,000 +/-2000 K, nominally placing it within the ZZ Ceti instability strip.

PY - 1992/8/1

Y1 - 1992/8/1

UR - https://ui.adsabs.harvard.edu/abs/1992ApJ...394L..53W/abstract

U2 - 10.1086/186470

DO - 10.1086/186470

M3 - Article

SN - 1538-4357

VL - 394

JO - The Astrophysical Journal

JF - The Astrophysical Journal

ER -

The binary system L151-81A/B : a potential test of accretion theory

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