Supernova remnants in the magellanic clouds

M. D. Filipovic; L. Staveley-Smith; W Reid; P. A. Jones

Supernova remnants in the magellanic clouds

M. D. Filipovic, L. Staveley-Smith, W Reid, P. A. Jones

Research output: Chapter in Book/Report/Conference proceeding › Conference proceeding contribution

Abstract

A study of the nature and the spatial distribution of over 250 discrete radio sources (HII regions and SNRs) in the Magellanic Clouds (MCs) is underway. A multi-frequency comparison of these sources involves the latest radio, IR, optical and X-ray surveys with angular resolution of <1'. Special emphasis is given to the MC SNRs. Their morphology, birth rate and overall properties are investigated and compared with Galactic SNRs and SNRs from other nearby galaxies. Also, we are investigating the radio source distribution throughout both MCs.

Original language	English
Title of host publication	Young neutron stars and their environments
Editors	Fernando Camilo
Place of Publication	San Francisco, CA
Publisher	Astronomical Society of the Pacific
Pages	87-88
Number of pages	2
ISBN (Print)	1583811788
Publication status	Published - 2004
Event	218th Symposium of the International-Astronomical-Union on Yound Neutron Stars and Their Environments - Sydney, Australia Duration: 14 Jul 2003 → 17 Jul 2003

Publication series

Name	IAU Symposia
Publisher	Astronomical Society of the Pacific
ISSN (Print)	0074-1809

Conference

Conference	218th Symposium of the International-Astronomical-Union on Yound Neutron Stars and Their Environments
Country/Territory	Australia
City	Sydney
Period	14/07/03 → 17/07/03

Cite this

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title = "Supernova remnants in the magellanic clouds",

abstract = "A study of the nature and the spatial distribution of over 250 discrete radio sources (HII regions and SNRs) in the Magellanic Clouds (MCs) is underway. A multi-frequency comparison of these sources involves the latest radio, IR, optical and X-ray surveys with angular resolution of <1'. Special emphasis is given to the MC SNRs. Their morphology, birth rate and overall properties are investigated and compared with Galactic SNRs and SNRs from other nearby galaxies. Also, we are investigating the radio source distribution throughout both MCs.",

author = "Filipovic, {M. D.} and L. Staveley-Smith and W Reid and Jones, {P. A.}",

year = "2004",

language = "English",

isbn = "1583811788",

series = "IAU Symposia",

publisher = "Astronomical Society of the Pacific",

pages = "87--88",

editor = "Fernando Camilo",

booktitle = "Young neutron stars and their environments",

note = "218th Symposium of the International-Astronomical-Union on Yound Neutron Stars and Their Environments ; Conference date: 14-07-2003 Through 17-07-2003",

}

Filipovic, MD, Staveley-Smith, L, Reid, W & Jones, PA 2004, Supernova remnants in the magellanic clouds. in F Camilo (ed.), Young neutron stars and their environments. IAU Symposia, Astronomical Society of the Pacific, San Francisco, CA, pp. 87-88, 218th Symposium of the International-Astronomical-Union on Yound Neutron Stars and Their Environments, Sydney, Australia, 14/07/03.

TY - GEN

T1 - Supernova remnants in the magellanic clouds

AU - Filipovic, M. D.

AU - Staveley-Smith, L.

AU - Reid, W

AU - Jones, P. A.

PY - 2004

Y1 - 2004

N2 - A study of the nature and the spatial distribution of over 250 discrete radio sources (HII regions and SNRs) in the Magellanic Clouds (MCs) is underway. A multi-frequency comparison of these sources involves the latest radio, IR, optical and X-ray surveys with angular resolution of <1'. Special emphasis is given to the MC SNRs. Their morphology, birth rate and overall properties are investigated and compared with Galactic SNRs and SNRs from other nearby galaxies. Also, we are investigating the radio source distribution throughout both MCs.

AB - A study of the nature and the spatial distribution of over 250 discrete radio sources (HII regions and SNRs) in the Magellanic Clouds (MCs) is underway. A multi-frequency comparison of these sources involves the latest radio, IR, optical and X-ray surveys with angular resolution of <1'. Special emphasis is given to the MC SNRs. Their morphology, birth rate and overall properties are investigated and compared with Galactic SNRs and SNRs from other nearby galaxies. Also, we are investigating the radio source distribution throughout both MCs.

M3 - Conference proceeding contribution

SN - 1583811788

T3 - IAU Symposia

SP - 87

EP - 88

BT - Young neutron stars and their environments

A2 - Camilo, Fernando

PB - Astronomical Society of the Pacific

CY - San Francisco, CA

T2 - 218th Symposium of the International-Astronomical-Union on Yound Neutron Stars and Their Environments

Y2 - 14 July 2003 through 17 July 2003

ER -

Supernova remnants in the magellanic clouds

Abstract

Publication series

Conference

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