z-logo
open-access-imgOpen Access
Spectroscopic variations of the Be star LQ And: binarity and rotation
Author(s) -
J. M. Matthews,
P. Harmanec,
G. A. H. Walker,
S. Yang,
W. H. Wehlau
Publication year - 1991
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/248.4.787
Subject(s) - physics , astrophysics , radial velocity , photometry (optics) , light curve , orbital period , spectral line , rotation period , stellar rotation , observable , be star , line (geometry) , galaxy rotation curve , star (game theory) , equivalent width , astronomy , emission spectrum , stars , geometry , galaxy , quantum mechanics , mathematics , halo

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

Address

John Eccles House
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom