Tidally compressed molecular gas in ultraluminous and early type galaxies

dc.contributor.author	Das, M
dc.contributor.author	Jog, C. J
dc.date.accessioned	2008-03-10T10:15:51Z
dc.date.available	2008-03-10T10:15:51Z
dc.date.issued	2000
dc.identifier.citation	BASI, Vol. 28, No. 2, pp. 389 - 391	en
dc.identifier.uri	http://hdl.handle.net/2248/2150
dc.description.abstract	The effect of the galactic tidal field is usually considered disruptive in the literature. However, in some cases its effect can become compressive. Using the virial theorem, we have determined the minimum density for a cloud to be stable and gravitationally bound within the tidally compressive region of a galaxy. We have applied our results to a sample of early type and ultraluminous galaxies observed in the literature. For early type galaxies with a core-type luminosity profile, the molecular gas is compressed to high densities of at least 104cm-3 within the inner 50 pc where the field is compressive. For ultraluminous galaxies our treatment predicts molecular gas densities of 102 - 104cm-3 within the central few 100 pc. These values agree well with gas densities observed in the centers of these galaxies.	en
dc.format.extent	167240 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/2000BASI...28..389D	en
dc.subject	Galaxies	en
dc.subject	Kinematics and dynamics-galaxies	en
dc.subject	ISM	en
dc.title	Tidally compressed molecular gas in ultraluminous and early type galaxies	en
dc.type	Article	en