Accretion Disks around low-mass Stars unveiled by the new Generation of cm to submm Arrays

Details Accretion Disks around low-mass Stars unveiled by the new Generation of cm to submm Arrays Accretion Disks around low-mass Stars unveiled by the new Generation of cm to submm Arrays

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010hia....15..239d&link_type=abstract

Highlights of Astronomy, Volume 15, p. 239-240

Astronomy and Astrophysics

Astronomy

Accretion Disks - Stars: Formation - Planetary Systems: Protoplanetary Disks

Scientific paper

In the context of accretion disks, I briefly discuss the impact of three major forthcoming radio facilities: e-VLA, ALMA and SKA. These arrays are complementary by their frequency range and angular resolution. Around nearby low-mass stars, they will likely provide the first insights in the inner gas and dust disks (radius < 10-30 AU) in the area where planet formation should occur but would also allow the first investigations of the star, jet and disk connections.

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