Sign on

SAO/NASA ADS Astronomy Abstract Service


· Find Similar Abstracts (with default settings below)
· Electronic Refereed Journal Article (HTML)
· On-line Data
· References in the article
· Citations to the Article (3) (Citation History)
· Refereed Citations to the Article
· Reads History
·
· Translate This Page
Title:
X-ray Detection from Shell-like SNR G359.1-0.5
Authors:
Yokogawa, J.; Sakano, M.; Koyama, K.; Yamauchi, S.
Affiliation:
AA(Department of Physics, Kyoto Univ., Kyoto 606-8502, Japan), AB(Department of Physics, Kyoto Univ., Kyoto 606-8502, Japan; Research Fellow of the Japan Society for the Promotion of Science, Japan), AC(Department of Physics, Kyoto Univ., Kyoto 606-8502, Japan; CREST: Japan Science and Technology Corporation (JST), Japan), AD(College of Humanities and Social Science, Iwate Univ., 3-18-34 Ueda, Morioka, Iwate 020-8550, Japan)
Publication:
Advances in Space Research, Volume 25, Issue 3-4, p. 571-574. (AdSpR Homepage)
Publication Date:
00/2000
Origin:
ELSEVIER
DOI:
10.1016/S0273-1177(99)00802-9
Bibliographic Code:
2000AdSpR..25..571Y

Abstract

We detected X-rays from the shell-like radio SNR (supernova remnant) G359.1-0.5 with ASCA satellite. Center-filled X-rays with no pulsation are found, but no X-ray from the radio shell is detected. The X-ray spectrum shows (1) a large absorption of 8× 1022 H cm-2, suggesting that G359.1-0.5 lies near the Galactic center, which is consistent with radio observations and (2) two prominent lines whose center energies correspond to the emission lines from He-like Si and H-like S. The line profile could be reproduced with a two-component plasma model, suggesting presence of a high temperature plasma together with an overabundance of S. No difference between emitting regions of the two components is found
Bibtex entry for this abstract   Preferred format for this abstract (see Preferences)

   

Find Similar Abstracts:

Use: Authors
Title
Abstract Text
Return: Query Results Return    items starting with number
Query Form
Database: Astronomy
Physics
arXiv e-prints