On infrared excess emission from HZ Herculis

dc.contributor.author	Ghosh, S. K.
dc.contributor.author	Iyengar, K. V. K.
dc.contributor.author	Verma, R. P.
dc.contributor.author	Srivastava, R. K.
dc.date.accessioned	2010-02-15T05:30:19Z
dc.date.available	2010-02-15T05:30:19Z
dc.date.issued	1989
dc.identifier.citation	This article downloded from ADS Free Online Journal	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/509
dc.description.abstract	In an attempt to confirm the recently observed 1.6 µm excess emission from RZ Her (Gnedin et al. 1986), we report negative results from observations made at identical binary phase. Implications of these measurements have been discussed in the light of 35 day cycles of Her X-1.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	ac a39-69
dc.subject	HZ Herculis	en_US
dc.title	On infrared excess emission from HZ Herculis	en_US
dc.type	Article	en_US