Spectral Classification: Old and Contemporary

Giridhar, S

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5412

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DC Field	Value	Language
dc.contributor.author	Giridhar, S	-
dc.date.accessioned	2011-03-10T10:33:45Z	-
dc.date.available	2011-03-10T10:33:45Z	-
dc.date.issued	2010	-
dc.identifier.citation	Goswami, A & Reddy, B. E., eds., Principles and Perspectives in Cosmochemistry, Lecture Notes on Kodai School on Synthesis of Elements in Stars, held at Kodaikanal Observatory, India April 29 –May 13, 2008, pp. 165-180	en
dc.identifier.uri	http://hdl.handle.net/2248/5412	-
dc.description	The original publication is available at springerlink.com	en
dc.description.abstract	Beginning with a historical account of the spectral classification, its refinement through additional criteria is presented. The line strengths and ratios used in two dimensional classifications of each spectral class are described. A parallel classification scheme for metal-poor stars and the standards used for classification are presented. The extension of spectral classification beyond M to L and T and spectroscopic classification criteria relevant to these classes are described. Contemporary methods of classifications based upon different automated approaches are introduced.	en
dc.language.iso	en	en
dc.publisher	Springer	en
dc.relation.uri	http://www.springerlink.com/content/tm3v2n5152415435/	en
dc.relation.uri	http://arxiv.org/abs/1003.4002	en
dc.rights	© Springer	en
dc.subject	Spectral classification	en
dc.subject	Luminosity classes	en
dc.subject	Metal-poor stars	en
dc.title	Spectral Classification: Old and Contemporary	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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