Spectrophotometric observations of Mira Ceti

dc.contributor.author	Joshi, S. C.
dc.contributor.author	Rautela, B. S.
dc.contributor.author	Sanwal, B. B.
dc.date.accessioned	2011-01-10T06:53:40Z
dc.date.available	2011-01-10T06:53:40Z
dc.date.issued	1980
dc.identifier.citation	This article is taken from ADS database	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/771
dc.description.abstract	Following an announcement in the IAU Circular No. 3407 by S. McLean, we have observed the long period variable Mira (o Ceti) on two nights (6 and 18 October 1979) with the help of a scanner attached to the 104-cm reflector of the Uttar Pradesh State Observatory as a spectral resolution of 50 A. The monochromatic magnitudes of the star have been corrected for atmospheric extinction and have been put on an absolute scale corresponding to Hayes and Latham (1975) calibration of Vega. Table 1 gives these data.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	ibvs1754
dc.subject	Mira Ceti	en_US
dc.title	Spectrophotometric observations of Mira Ceti	en_US
dc.type	Article	en_US