Observations of weak G-band stars

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