Dust in the Local Group View Full Text


Ontology type: schema:Chapter      Open Access: True


Chapter Info

DATE

2014-11-14

AUTHORS

Aigen Li , Shu Wang , Jian Gao , B. W. Jiang

ABSTRACT

How dust absorbs and scatters starlight as a function of wavelength (known as the interstellar extinction curve) is crucial for correcting for the effects of dust extinction in inferring the true luminosity and colors of reddened astrophysical objects. Together with the extinction spectral features, the extinction curve contains important information about the dust size distribution and composition. This review summarizes our current knowledge of the dust extinction of the Milky Way, three Local Group galaxies (i.e., the Small and Large Magellanic Clouds, and M 31), and galaxies beyond the Local Group. More... »

PAGES

85-103

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/978-3-319-10614-4_8

DOI

http://dx.doi.org/10.1007/978-3-319-10614-4_8

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1021936491


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