Published July 1975 | Version v1
Journal article

Do comets play a role in galactic chemistry and γ-ray bursts

Creators

  • 1. Center for Astrophysics, Harvard College Observatory and Smithsonian Astrophysical Observatory, Cambridge, Massachusetts 02138

Description

This paper explores the plausibility of the assumption that enough material from interstellar space is locked up in comets to reduce significantly the apparent growth rate of ''heavy'' elements (mass greater than H/sube/) and, therefore, the present abundance of heavy elements in the interstellar medium and in the disk stars. A related suggestion concerns the influx of comets on neutron stars as a source of γ-ray bursts. Although no interstellar comets have been observed, reasonable upper limits to the observed numbers and masses do not rule out the first suggestion. The γ-ray-burst suggestion appears unlikely. A surprisingly large total mass of comets could be gravitationally bound to the Sun and, of course, to other stars, but remain undetected. The nature of the 1908 Tunguska explosion is discussed briefly. It was probably not an encounter with an active comet

Additional details

Identifiers

Publishing Information

Journal Title
The Astronomical Journal
Journal Volume
80
Journal Issue
7
Series
Astron. J.
Journal Page Range
525
ISSN
0004-6256

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
6211789
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
CHEMICAL COMPOSITION; COMETS; COSMIC GAMMA SOURCES; GALACTIC EVOLUTION; NEUTRON STARS; SOLAR SYSTEM
Descriptors DEC
COSMIC RAY SOURCES; STARS

Optional Information

Notes
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