SNRs in M33 from optical and X-ray (Long+, 2010)

Details SNRs in M33 from optical and X-ray (Long+, 2010) SNRs in M33 from optical and X-ray (Long+, 2010)

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ycat..21870495l&link_type=abstract

VizieR On-line Data Catalog: J/ApJS/187/495. Originally published in: 2010ApJS..187..495L

Computer Science

Galaxies: Optical, X-Ray Sources, Supernova Remnants, Morphology

Scientific paper

The strategy for the ChASeM33 survey has been described in detail by Plucinsky et al. (2008, Cat. J/ApJS/174/366). The survey comprises ACIS-I observations of seven overlapping fields which cover the inner region of M33 to a radius of about 18', or 4.3kpc. Data include not only those obtained by us as part of ChASeM33, between 2005 September and 2006 November, but also ACIS-I data from observations which are available from the Chandra archive (ObsIDs 1730 and 2023). Optical spectroscopy was used in support of the Chandra SNR analysis (see Note 6 of Table 3).
(2 data files).

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