Disks and Outflows

Details Disks and Outflows Disks and Outflows

May 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aas...200.5110r&link_type=abstract

American Astronomical Society, 200th AAS Meeting, #51.10; Bulletin of the American Astronomical Society, Vol. 34, p.725

Astronomy and Astrophysics

Astronomy

1

Scientific paper

The presence of disks and outflows characterizes the earliest stages of stellar evolution. I will review recent results that exemplify how the radio observations have become powerful tools in the study of these extremely young objects. Binarity and multiplicity seem to be factors that we are only starting to understand. Outflows are now seen as laboratories for the chemistry of shocked regions. Finally, the efforts to extend the paradigm for low-mass stellar formation to more massive protostars can be tested critically in the radio wavelengths. I acknowledge the support from CONACyT, Mexico.

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