Elemental abundance analyses with DAO spectrograms. – XXVI. The superficially normal stars gamma Serpentis (F6 V) and 101 Herculis (A7 V)

dc.contributor.author	TEKTUNALI, H. GÖKMEN
dc.contributor.author	ÇAY, İPEK
dc.contributor.author	Yelkenci, Ayşegül
dc.contributor.author	ÇALIŞKAN, HÜLYA
dc.contributor.author	ÇAY, MEHMET TAŞKIN
dc.contributor.author	Adelman, Saul J.
dc.contributor.author	Gulliver, A. F.
dc.contributor.author	Koçer, Dursun
dc.date.accessioned	2021-03-04T11:50:23Z
dc.date.available	2021-03-04T11:50:23Z
dc.identifier.citation	ÇALIŞKAN H., Adelman S. J. , ÇAY M. T. , ÇAY İ., Gulliver A. F. , TEKTUNALI H. G. , Koçer D., Yelkenci A., "Elemental abundance analyses with DAO spectrograms. – XXVI. The superficially normal stars gamma Serpentis (F6 V) and 101 Herculis (A7 V)", A&A, cilt.394, 2002
dc.identifier.other	vv_1032021
dc.identifier.other	av_745b0a77-b9a3-4248-b55f-dd4f9e5055d8
dc.identifier.uri	http://hdl.handle.net/20.500.12627/79974
dc.identifier.uri	http://adsabs.harvard.edu/abs/2002A%26A...394..187C
dc.language.iso	eng
dc.title	Elemental abundance analyses with DAO spectrograms. – XXVI. The superficially normal stars gamma Serpentis (F6 V) and 101 Herculis (A7 V)
dc.type	Makale
dc.relation.journal	A&A
dc.contributor.department	, ,
dc.identifier.volume	394
dc.contributor.firstauthorID	472155

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