Observations of weak G-band stars

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4074

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DC Field	Value	Language
dc.contributor.author	Kameswara Rao, N	-
dc.date.accessioned	2008-12-16T14:21:03Z	-
dc.date.available	2008-12-16T14:21:03Z	-
dc.date.issued	1978-11	-
dc.identifier.citation	Monthly Notices Royal Astronomical Society, Vol. 185, pp. 585 - 589	en
dc.identifier.issn	0035-8711 (Print) 1365-2966 (Online)	-
dc.identifier.uri	http://hdl.handle.net/2248/4074	-
dc.description	Open Access	-
dc.description.abstract	Scanner observations of the strengths of the G-band stars of CH at λ4300 and of the NH bands at λ3360 were obtained fro 10 weak G-band stars (wG stars) along with 2 normal field giants of spectral types G to K. the differential strengths of these in wG stars relative to the field giants show that the weakness of the G band is linearly related to the enhancement of the NH band strength thus showing that the atmospheric material of the wG stars is processed by the CNO cycle.	en
dc.language.iso	en	en
dc.publisher	Royal Astronomical Society	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1978MNRAS.185..585R	en
dc.relation.uri	http://www3.interscience.wiley.com/journal/117974593/toc?func=showIssues&code=mnr	-
dc.rights	©Royal Astronomical Society	-
dc.subject	G-Band Stars	en
dc.subject	Spectra	-
dc.title	Observations of weak G-band stars	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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