z-logo
open-access-imgOpen Access
The orbit of the supergiant component of Vela X-1 derived from IUE radial velocities
Author(s) -
D. J. Stickland,
C. Lloyd,
A. Radziun-Woodham
Publication year - 1997
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/286.2.l21
Subject(s) - physics , vela , supergiant , astrophysics , neutron star , radial velocity , astronomy , spectral line , circular orbit , pulsar , stars

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