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A Reference Sample: ISM of the Most Isolated Galaxies

Published online by Cambridge University Press:  26 May 2016

L. Verdes-Montenegro
Affiliation:
Instituto de Astrofísica de Andalucía-CSIC, Granada, Spain
J. Sulentic
Affiliation:
Physics & Astronomy, University of Alabama, USA
D. Espada
Affiliation:
Instituto de Astrofísica de Andalucía-CSIC, Granada, Spain
S. Leon
Affiliation:
Instituto de Astrofísica de Andalucía-CSIC, Granada, Spain
U. Lisenfeld
Affiliation:
Instituto de Astrofísica de Andalucía-CSIC, Granada, Spain
S. Verley
Affiliation:
Instituto de Astrofísica de Andalucía-CSIC, Granada, Spain
W. Huchtmeier
Affiliation:
Max-Planck-Institut für Radioastronomie, Bonn, Germany
S. Odewahn
Affiliation:
Department of Physics and Astronomy, Arizona State University, USA
E. Garcia
Affiliation:
Instituto de Astrofísica de Andalucía-CSIC, Granada, Spain
M. S. Yun
Affiliation:
Department of Physics and Astronomy, University of Massachusetts, USA
S. del Río
Affiliation:
INAOE, Puebla, Mexico
F. Combes
Affiliation:
Observatoire de Paris - LERMA, France

Abstract

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We are constructing the first complete unbiased control sample of the most isolated galaxies of the northern sky to serve as a template in the study of star formation and galaxy evolution in denser environments. Our goal is to compare and quantify the properties of different phases of the interstellar medium in this sample, as well as the level of star formation, both relevant parameters in the internal evolution of galaxies and strongly conditioned by the environment. To achieve this goal we are building a multiwavelength database for this sample to compare and quantify the properties of different phases of the ISM.

Type
Part 2. Origin
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

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Verdes-Montenegro, L., Sempere, M. J., Sulentic, J., & Cernicharo, J. 2001, ESASP, 460, 515.Google Scholar
Verdes-Montenegro, L., Sauvage, M., Sempere, M. J., Sulentic, J., & Cernicharo, J., 2002, AP&SS, 281, 1, 427.Google Scholar