Does the LFIR-LHCN correlation hold for low LFIR isolated galaxies?

Ocaña Flaquer, Breezy; Leon, S.; Espada Fernández, Daniel; Martín Ruiz, Sergio; Lisenfeld , Ute; Verley, Simon; Sabater, J.; Verdes-Montenegro, L.

Ocaña_IsolatedGalaxies.pdf (62.03Kb)

Identificadores

URI: http://hdl.handle.net/10481/28387

ISSN: 1050-3390

ISBN: 978-1-58381-722-3

ISBN: 978-1-58381-723-0

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Editorial

Astronomical Society of the Pacific

Materia

Isolated

Galaxies

Fecha

2009

Referencia bibliográfica

Ocaña Flaquer, B.; et al. Does the LFIR-LHCN correlation hold for low LFIR isolated galaxies?. In: Verdes-Montenegro, L; Olmo, A. y Sulentic, J. (eds.) Galaxies in Isolation: exploring nature versus nature. San Francisco (USA): Astronomical Society of the Pacific, 2010. p. 274. (Conference Series, 421). [http://hdl.handle.net/10481/28387]

Resumen

Low LFIR Isolated Galaxies (IGs) from the AMIGA sample have low level of Star Formation (SF) activity. We observed the HCN(1-0) emission in a sample of IGs in order to test whether they follow the tight relation between LHCN and LFIR found for galaxies with more active SF.

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