Modeling the Dust Emission of the L 1551 IRS 5 Binary System at Different Scales

Details Modeling the Dust Emission of the L 1551 IRS 5 Binary System at Different Scales Modeling the Dust Emission of the L 1551 IRS 5 Binary System at Different Scales

Jan 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003rmxac..15..142o&link_type=abstract

Winds, Bubbles, and Explosions: a conference to honor John Dyson, Pátzcuaro, Michoacán, México, September 9-13, 2002 (Eds. S. J.

Astronomy and Astrophysics

Astronomy

Accretion, Accretion Disk, Binaries: Close, Ism: Individual (L 1551 Irs 5), Radiative Transfer, Stars: Formation

Scientific paper

We present a self-consistent model to investigate the physical
properties on different scales of the circumstellar material around the
Class I source L 1551 IRS 5.

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