Dynamical infall around low-mass protostar candidates.

Details Dynamical infall around low-mass protostar candidates. Dynamical infall around low-mass protostar candidates.

Nov 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996asthe..89..492o&link_type=abstract

Astronomical Herald, Vol. 89, No. 11, p. 492 - 499

Astronomy and Astrophysics

Astronomy

Protostars: Accretion

Scientific paper

Dynamical infall is an essential phenomenon in star formation. Although dynamical infall has been veiled for a long time because of its small velocity and size, recent high sensitivity interferometers enable to observe dynamical infall directly. The author reports recent observations of dynamical infall around low-mass, i.e., solar-type protostar candidates with the Nobeyama Millimeter Array.

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