Searching for Young Type Ia Supernova Remnants in M83

Chuan Jui Li; You Hua Chu; Po Sheng Ou

doi:10.1017/S1743921317004835

Searching for Young Type Ia Supernova Remnants in M83

Chuan Jui Li, You Hua Chu, Po Sheng Ou

Astronomy

Research output: Contribution to journal › Article › peer-review

Abstract

Young Type Ia supernova remnants (SNRs) are characterized by Balmer-dominated optical spectra, well-defined shell morphologies, > 10³⁶ ergs s^-1 X-ray luminosities, and a lack of massive stars and dense interstellar gas in their vicinity. Applying these characteristics and using archival deep HST and Chandra observations of M83, we search for young Type Ia SNRs in this spiral galaxy. This is a very difficult task!.

Original language	English (US)
Pages (from-to)	213-215
Number of pages	3
Journal	Proceedings of the International Astronomical Union
Volume	12
Issue number	S331
DOIs	https://doi.org/10.1017/S1743921317004835
State	Published - Feb 1 2017

Keywords

ISM: supernova remnants

ASJC Scopus subject areas

Medicine (miscellaneous)
Astronomy and Astrophysics
Nutrition and Dietetics
Public Health, Environmental and Occupational Health
Space and Planetary Science

Online availability

10.1017/S1743921317004835

Library availability

Discover UIUC Full Text

Cite this

@article{b33f8d07067e4fb7a5444efea835fcb5,

title = "Searching for Young Type Ia Supernova Remnants in M83",

abstract = "Young Type Ia supernova remnants (SNRs) are characterized by Balmer-dominated optical spectra, well-defined shell morphologies, > 1036 ergs s-1 X-ray luminosities, and a lack of massive stars and dense interstellar gas in their vicinity. Applying these characteristics and using archival deep HST and Chandra observations of M83, we search for young Type Ia SNRs in this spiral galaxy. This is a very difficult task!.",

keywords = "ISM: supernova remnants",

author = "Li, {Chuan Jui} and Chu, {You Hua} and Ou, {Po Sheng}",

note = "Funding Information: This project is supported by MoST grant 104-2112-M001-044-MY3. Publisher Copyright: {\textcopyright} 2017 International Astronomical Union.",

year = "2017",

month = feb,

day = "1",

doi = "10.1017/S1743921317004835",

language = "English (US)",

volume = "12",

pages = "213--215",

journal = "Proceedings of the International Astronomical Union",

issn = "1743-9213",

publisher = "Cambridge University Press",

number = "S331",

}

TY - JOUR

T1 - Searching for Young Type Ia Supernova Remnants in M83

AU - Li, Chuan Jui

AU - Chu, You Hua

AU - Ou, Po Sheng

PY - 2017/2/1

Y1 - 2017/2/1

N2 - Young Type Ia supernova remnants (SNRs) are characterized by Balmer-dominated optical spectra, well-defined shell morphologies, > 1036 ergs s-1 X-ray luminosities, and a lack of massive stars and dense interstellar gas in their vicinity. Applying these characteristics and using archival deep HST and Chandra observations of M83, we search for young Type Ia SNRs in this spiral galaxy. This is a very difficult task!.

AB - Young Type Ia supernova remnants (SNRs) are characterized by Balmer-dominated optical spectra, well-defined shell morphologies, > 1036 ergs s-1 X-ray luminosities, and a lack of massive stars and dense interstellar gas in their vicinity. Applying these characteristics and using archival deep HST and Chandra observations of M83, we search for young Type Ia SNRs in this spiral galaxy. This is a very difficult task!.

KW - ISM: supernova remnants

UR - http://www.scopus.com/inward/record.url?scp=85047168062&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85047168062&partnerID=8YFLogxK

U2 - 10.1017/S1743921317004835

DO - 10.1017/S1743921317004835

M3 - Article

AN - SCOPUS:85047168062

SN - 1743-9213

VL - 12

SP - 213

EP - 215

JO - Proceedings of the International Astronomical Union

JF - Proceedings of the International Astronomical Union

IS - S331

ER -

Searching for Young Type Ia Supernova Remnants in M83

Abstract

Keywords

ASJC Scopus subject areas

Online availability

Library availability

Related links

Fingerprint

Cite this