Cold gas at high redshifts

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DC Field	Value	Language
dc.contributor.author	Bagla, J.S.	-
dc.date.accessioned	2021-07-13T06:20:57Z	-
dc.date.available	2021-07-13T06:20:57Z	-
dc.date.issued	2013	-
dc.identifier.citation	31st ASI Meeting, ASI Conference Series, 2013, Vol. 9, p. 85	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/3699	-
dc.identifier.uri	http://cdsads.u-strasbg.fr/pdf/2013ASInC...9...85B	-
dc.description	Only IISERM authors are available in the record.	en_US
dc.description.abstract	I will discuss the use of semi analytic models of galaxy formation for calculating the cold gas fraction in galaxies. I will apply this to compute the large scale distribution of cold gas at high redshifts and comment on observability of the signal using upgraded and upcoming radio telescopes.	en_US
dc.language.iso	en	en_US
dc.publisher	ASI Conference Series	en_US
dc.subject	Cold Gas	en_US
dc.subject	Galaxy formation	en_US
dc.title	Cold gas at high redshifts	en_US
dc.type	Article	en_US
Appears in Collections:	Research Articles

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