Sign on

SAO/NASA ADS Astronomy Abstract Service

· Find Similar Abstracts (with default settings below)
· Full Refereed Journal Article (PDF/Postscript)
· Full Refereed Scanned Article (GIF)
· References in the article
· Citations to the Article (15) (Citation History)
· Refereed Citations to the Article
· SIMBAD Objects (1)
· Also-Read Articles (Reads History)
·
· Translate This Page
Title:
A new radio map of the AD 1006 supernova remnant, G327.6 + 14.6
Authors:
Caswell, J. L.; Haynes, R. F.; Milne, D. K.; Wellington, K. J.
Affiliation:
AA(Commonwealth Scientific and Industrial Research Organization, Div. of Radiophysics, Epping, New South Wales, Australia), AB(Commonwealth Scientific and Industrial Research Organization, Div. of Radiophysics, Epping, New South Wales, Australia), AC(Commonwealth Scientific and Industrial Research Organization, Div. of Radiophysics, Epping, New South Wales, Australia), AD(Commonwealth Scientific and Industrial Research Organization, Div. of Radiophysics, Epping, New South Wales, Australia)
Publication:
Royal Astronomical Society, Monthly Notices (ISSN 0035-8711), vol. 204, Sept. 1983, p. 921-926. (MNRAS Homepage)
Publication Date:
09/1983
Category:
Astronomy
Origin:
STI
NASA/STI Keywords:
ASTRONOMICAL MAPS, RADIO SPECTRA, STELLAR ENVELOPES, SUPERNOVA REMNANTS, EMISSION SPECTRA, SPECTRAL RESOLUTION, STELLAR MASS EJECTION, VISIBLE SPECTRUM, X RAY SPECTRA
Bibliographic Code:
1983MNRAS.204..921C

Abstract

The radio remnant of the AD 1006 supernova has been mapped with resolution of ≡1 arcmin. The radio map and a recent X-ray map of similar resolution both show a bright ring of emission indicative of a shell structure. While the general appearance is remarkably similar, with both radio and X-ray emission strong in the same general portions of the ring, detailed comparisons show no precise correspondence of the brightest features. A major difference is that the X-ray emission is quite intense at the centre of the ring, where there is essentially no detectable radio emission. Optical observations conflict with the X-ray interpretation of a large ejected mass, high energy and no deceleration to date.

Printing Options

Print whole paper
Print Page(s) through

Return 600 dpi PDF to Acrobat/Browser. Different resolutions (200 or 600 dpi), formats (Postscript, PDF, etc), page sizes (US Letter, European A4, etc), and compression (gzip,compress,none) can be set through the Printing Preferences


More Article Retrieval Options

HELP for Article Retrieval
Bibtex entry for this abstract   Preferred format for this abstract (see Preferences)
   

Find Similar Abstracts:

Use: Authors
Title
Keywords (in text query field)
Abstract Text
Return: Query Results Return    items starting with number
Query Form
Database: Astronomy
Physics
arXiv e-prints