Published November 1, 1975 | Version v1
Journal article Metadata-only

Variable stars in the x-ray globular cluster NGC 1851

Creators

  • 1. Harvard College Observatory and Smithsonian Astrophysical Observatory, Cambridge, MA

Description

Ten known and four new variable stars in the X-ray globular cluster NGC 1851 have been studied. None of these variables show obvious unusual characteristics that would make them candidates for the X-ray emission. The characteristics of the variable stars are presented

Additional details

Identifiers

DOI
10.1086/181957;

Publishing Information

Journal Title
The Astrophysical Journal
Journal Volume
201
Journal Issue
3
Series
Astrophys. J., Lett.
Journal Page Range
L125
ISSN
0004-637X

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
7247005
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
BRIGHTNESS; COSMIC X-RAY SOURCES; STAR CLUSTERS; VARIABLE STARS; VARIATIONS; VISIBLE RADIATION
Descriptors DEC
COSMIC RAY SOURCES; ELECTROMAGNETIC RADIATION; OPTICAL PROPERTIES; PHYSICAL PROPERTIES; RADIATIONS; STARS

Optional Information

Notes
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