A 0.24+0.18 M⊙ double-lined eclipsing binary from the HATSouth survey | Zendy

George Zhou | Zendy; D. Bayliss | Zendy; J. D. Hartman | Zendy; M. Rabus | Zendy; G. Á. Bakos | Zendy; Andrés Jordán | Zendy; Rafael Brahm | Zendy; K. Penev | Zendy; Z. Csubry | Zendy; L. Mancini | Zendy; Néstor Espinoza | Zendy; M. de Val-Borro | Zendy; W. Bhatti | Zendy; S. Ciceri | Zendy; T. Henning | Zendy; B. Schmidt | Zendy; Simon J. Murphy | Zendy; R. Paul Butler | Zendy; P. Arriagada | Zendy; Stephen A. Shectman | Zendy; Jeffrey D. Crane | Zendy; I. Thompson | Zendy; V. Suc | Zendy; R. W. Noyes | Zendy

AI Assistant Blog Pricing

Home ZAIA Blog

Open Access

A 0.24+0.18 M⊙ double-lined eclipsing binary from the HATSouth survey

Author(s) -

George Zhou,

D. Bayliss,

J. D. Hartman,

M. Rabus,

G. Á. Bakos,

Andrés Jordán,

Rafael Brahm,

K. Penev,

Z. Csubry,

L. Mancini,

Néstor Espinoza,

M. de Val-Borro,

W. Bhatti,

S. Ciceri,

T. Henning,

B. Schmidt,

Simon J. Murphy,

R. Paul Butler,

P. Arriagada,

Stephen A. Shectman,

Jeffrey D. Crane,

I. Thompson,

V. Suc,

R. W. Noyes

Publication year - 2015

Publication title -

monthly notices of the royal astronomical society

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 2.058

H-Index - 383

eISSN - 1365-8711

pISSN - 0035-8711

DOI - 10.1093/mnras/stv1070

Subject(s) - physics , astrophysics , eclipse , context (archaeology) , radius , effective temperature , binary number , stars , brown dwarf , binary star , orbital period , radial velocity , stellar mass , star formation , arithmetic , mathematics , paleontology , computer security , computer science , biology

We report the discovery and characterization of a new M-dwarf binary, with component masses and radii of $M_1 = 0.244_{-0.003}^{+0.003} \, \mathrm{M}_{\odot }$, $R_1 = 0.261_{-0.009}^{+0.006} \, \mathrm{R}_{\odot }$, $M_2 = 0.179_{-0.001}^{+0.002} \, \mathrm{M}_{\odot }$, $R_2 = 0.218 _{-0.011}^{+0.007} \, \mathrm{R}_{\odot }$, and orbital period of ∼4.1 d. The M-dwarf binary HATS551−027 (LP 837−2...

The content you want is available to Zendy users.

Already have an account? Click here to sign in.

Having issues? You can contact us here

Accelerating Research