dc.contributor.author |
Mallik, D. C. V |
|
dc.date.accessioned |
2005-02-09T02:01:56Z |
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dc.date.available |
2005-02-09T02:01:56Z |
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dc.date.issued |
1982-06 |
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dc.identifier.citation |
BASI, Vol. 10, No. 2, pp. 73-110 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/332 |
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dc.description |
Open Access |
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dc.description.abstract |
Recent research on planetary nebulae is reviewed, with special emphasis on ultraviolet and infrared observations. Various distance scales and statistics based on them are discussed and the emperical mass-radius relation due to Maciel & Pottasch (1980) is used to compile a new list of local planetaries. Recent determinations of the effective temperatures of central stars and their new locations onthe H-R diagram are described. The implications of the chemical abundance studies of these nebulae are discussed in the light of current work on stellar evolution and nucleosynthesis. |
en |
dc.format.extent |
4093217 bytes |
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dc.format.mimetype |
application/pdf |
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dc.language.iso |
en |
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dc.publisher |
Astronomical Society of India |
en |
dc.subject |
Planetary Nebulae Statistics |
en |
dc.subject |
Abundances |
en |
dc.subject |
Stellar Evolution |
en |
dc.title |
Planetary nebulae |
en |
dc.type |
Article |
en |