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Radial distribution of (Fe X) and (Fe XIV) emission in the Cygnus Loop. II

Journal Article · · Astrophys. J.; (United States)
DOI:https://doi.org/10.1086/157689· OSTI ID:5364315
; ; ;
The radial distribution of (Fe X) and (Fe XIV) are now available for two regions in the northeast and west parts of the Cygnus Loop. The implications of these measurements for temperature, density, and shock history of the supernova remnant, and their relation to X-ray observations are discussed.
Research Organization:
Code 681, Laboratory for Astronomy and Solar Physics, Goddard Space Flight Center, Greenbelt, Maryland
OSTI ID:
5364315
Journal Information:
Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 235:3; ISSN ASJOA
Country of Publication:
United States
Language:
English

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Related Subjects

640103* -- Astrophysics & Cosmology-- Quasi-Stellar
Radio
& X-Ray Sources-- (-1987)
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ATOMIC IONS
CHARGED PARTICLES
COSMIC GASES
COSMIC RADIO SOURCES
COSMIC RAY SOURCES
COSMIC X-RAY SOURCES
DENSITY
DISTRIBUTION
EMISSION SPECTRA
FLUIDS
GASES
IONS
IRON IONS
NEBULAE
PHYSICAL PROPERTIES
SPATIAL DISTRIBUTION
SPECTRA
SUPERNOVA REMNANTS
TEMPERATURE DISTRIBUTION