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http://hdl.handle.net/2248/757Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Tej, A | - |
| dc.contributor.author | Lancon, A | - |
| dc.contributor.author | Scholz, M | - |
| dc.date.accessioned | 2006-03-14T05:17:29Z | - |
| dc.date.available | 2006-03-14T05:17:29Z | - |
| dc.date.issued | 2005-06 | - |
| dc.identifier.citation | BASI, Vol. 33, No. 2, pp. 103-108 | en |
| dc.identifier.uri | http://hdl.handle.net/2248/757 | - |
| dc.description.abstract | For stars with atmospheres as complex as those of Miras, determination of fundamental stellar parameters remains a challenge. Occurrence of water "shells" and their implication on the interpretation of the angular diameter measurements will be discussed in this talk. The role of a spectrophotometric index of water in estimating the continuum diameter will be highlighted. | en |
| dc.format.extent | 196863 bytes | - |
| dc.format.mimetype | application/pdf | - |
| dc.language.iso | en | en |
| dc.publisher | Astronomical Society of India | en |
| dc.subject | Stars | en |
| dc.subject | fundamental parameters - Stars | en |
| dc.subject | late-type - Stars | en |
| dc.subject | variable: general - Stars | en |
| dc.title | Interpretation of angular diameter measurements of Mira variables: role of water | en |
| dc.type | Article | en |
| Appears in Collections: | BASI Publications | |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| 0533103.PDF | 192.25 kB | Adobe PDF | ![]() View/Open |
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