| dc.contributor.author | Saxena, B. K | |
| dc.contributor.author | Srivastava, R. K | |
| dc.date.accessioned | 2007-10-19T11:29:26Z | |
| dc.date.available | 2007-10-19T11:29:26Z | |
| dc.date.issued | 1997 | |
| dc.identifier.citation | BASI, Vol. 25, No. 1, pp. 103 - 116 | en |
| dc.identifier.uri | http://hdl.handle.net/2248/1913 | |
| dc.description.abstract | The first observations of n Hya, taken at Pachmarhi, are presented. Night to night light variability on n Hya has been discussed. Maximum amplitude of light variation is found to be 0m 096. Preliminary results show that semi-regular variations with period around 0d.1 are present. The colour of n Hya has also been estimated. | en |
| dc.format.extent | 639117 bytes | |
| dc.format.mimetype | application/pdf | |
| dc.language.iso | en | en |
| dc.publisher | Astronomical Society of India | en |
| dc.relation.uri | http://adsabs.harvard.edu/abs/1997BASI...25..103S | en |
| dc.subject | Photoelectric | en |
| dc.subject | Photometry | en |
| dc.subject | Variable star | en |
| dc.title | Variability of eta Hydrae | en |
| dc.type | Article | en |