dc.contributor.author |
Bhatt, H. C |
|
dc.date.accessioned |
2004-11-08T11:21:36Z |
|
dc.date.available |
2004-11-08T11:21:36Z |
|
dc.date.issued |
1988 |
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dc.identifier.citation |
Kodaikanal Observatory Bulletins Series A, Vol 10, pp. 33-41 |
en |
dc.identifier.issn |
0374-3632 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/4 |
|
dc.description.abstract |
Results obtained from infrared observations of SN 1987A have been summarized. The supernova developed near-infrared excesses with a characteristic temperature ~1250 k beginning around March 15, 1987. Infrared speckle interferometry began to partially resolve the supernova from mid-June, and on August 6 a fully resolved structure (~0.42 arc second) was observed: consistent only with a light echo. Infrared spectroscopy in early October showed that all the lines and the molecular CO bands were redshifted with respect to the LMC by ~ 400-1500 km/sec. The dust responsible for the infrared light echo is expected to thermally reemit at far-infrared wavelengths (~30µm) which should be looked for. |
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dc.format.extent |
222421 bytes |
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dc.format.mimetype |
application/pdf |
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dc.language.iso |
en_US |
|
dc.publisher |
Indian Institute of Astrophysics |
en |
dc.subject |
Supernova 1987A |
en |
dc.subject |
Infrared Observations |
en |
dc.title |
Supernova 1987A in LMC : Infrared Observations |
en |
dc.type |
Article |
en |