Published 1990 | Version v1
Book

A new boundary for the Vela supernova remnant

Creators

  • 1. Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (USA)

Description

The Vela supernova remnant (SNR), at a distance of 0.5 kpc, is one of the closest SNR to Earth. It was first detected as a conglomerate of radio sources, Vela X, Y, and Z. The remnant was surveyed with the Einstein Imaging Proportional Counter (IPC) in 1979-80. 33 fields covered the Vela XYZ radio source. The resultant merged x-ray image shows the rim of the remnant in the north and east, fades below threshold in the west, and in the south, the boundary extends beyond the observed region. This paper describes the Vela SNR from these observations. (author)

Additional details

Publishing Information

Publisher
Cambridge University Press.
Imprint Place
Cambridge (UK)
ISBN
0 521 38105 3
Imprint Title
Imaging X-ray astronomy: a decade of Einstein Observatory achievements
Imprint Pagination
348 p.
Journal Page Range
p. 241-245.

Conference

Title
a decade of Einstein Observatory achievements.
Acronym
Symposium on imaging X-ray astronomy
Dates
13-15 Nov 1988.
Place
Cambridge, MA (USA).

INIS

Country of Publication
United Kingdom
Country of Input or Organization
United Kingdom
INIS RN
22036136
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Conference
Descriptors DEI
GAMMA ASTRONOMY; IMAGE SCANNERS; SUPERNOVA REMNANTS; TELESCOPES; X-RAY DETECTION; X-RAY SPECTROSCOPY
Descriptors DEC
ASTRONOMY; COSMIC RADIO SOURCES; DETECTION; RADIATION DETECTION; SPECTROSCOPY

Optional Information

Contract/Grant/Project number
Contract NAS8-30751; JPL957636