Published January 15, 1977 | Version v1
Journal article Metadata-only

Radio emission from AG Pegasi

Creators

  • 1. Physics Department and Institute of Astronomy, University of British Columbia

Description

Radio emission from the symbiotic nova AG Pegasi has been detected at 2.8 and 3.7 cm, and an upper limit has been obtained at 11 cm. The observations are interpreted as free-free emission from an ionized nebula formed by continuous mass ejection from the hot star. Our observations indicate a mass loss rate of 10-6 M/sub sun/ yr-1 and a total mass for the nebula of 7 x 10-5 M/sub sun/

Additional details

Identifiers

DOI
10.1086/154948;

Publishing Information

Journal Title
The Astrophysical Journal
Journal Volume
211
Journal Issue
2
Series
Astrophys. J.
Journal Page Range
429
ISSN
0004-637X

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
8326645
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
BINARY STARS; COSMIC RADIO SOURCES; NOVAE; PLANETARY NEBULAE; RADIOWAVE RADIATION; STAR MODELS; VARIABLE STARS
Descriptors DEC
ELECTROMAGNETIC RADIATION; MATHEMATICAL MODELS; NEBULAE; RADIATIONS; STARS

Optional Information

Notes
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