X-ray detection of SN1994W in NGC 4041?

Authors
Citation
Em. Schlegel, X-ray detection of SN1994W in NGC 4041?, ASTROPHYS J, 527(2), 1999, pp. L85-L88
Citations number
30
Categorie Soggetti
Space Sciences
Journal title
ASTROPHYSICAL JOURNAL
ISSN journal
0004637X → ACNP
Volume
527
Issue
2
Year of publication
1999
Part
2
Pages
L85 - L88
Database
ISI
SICI code
0004-637X(199912)527:2<L85:XDOSIN>2.0.ZU;2-X
Abstract
Optical spectra of SN 1994W in NGC 4041 revealed the presence of a dense (N -e > 10(8) cm(-3)) circumstellar shell. An observation with the ROSAT High- Resolution Imager detected a source, with a luminosity of similar to 8 x 10 (39) ergs s(-1), coincident with the position of SN 1994W to within 1".4. T he positional coincidence plus the optical evidence for a dense circumstell ar shell support the identification of the X-ray source as SN 1994W.