A comparative study of two globules from optical to far-infrared wavelengths

Details A comparative study of two globules from optical to far-infrared wavelengths A comparative study of two globules from optical to far-infrared wavelengths

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005esasp.577..379l&link_type=abstract

In: Proceedings of the dusty and molecular universe: a prelude to Herschel and ALMA, 27-29 October 2004, Paris, France. Ed. by A

Mathematics

Logic

Ism: Clouds, Dust, Extinction, Infrared: Ism

Scientific paper

We present observations of two morphologically similar globules, one of which has star formation, while the other has not. Optical and near-IR surface brightness observations, together with extinction measurements of background stars are used to study the radial density distributions of the clouds. Far-infrared observations made with ISO are used to study the properties of dust in these clouds.

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