BIMA Observations of B335 and L1527, Two Class 0 Collapsing Protostars

Details BIMA Observations of B335 and L1527, Two Class 0 Collapsing Protostars BIMA Observations of B335 and L1527, Two Class 0 Collapsing Protostars

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aas...193.7210e&link_type=abstract

American Astronomical Society, 193rd AAS Meeting, #72.10; Bulletin of the American Astronomical Society, Vol. 30, p.1360

Astronomy and Astrophysics

Astronomy

Scientific paper

We have observed B335 and L1527, two Class 0 sources with strong evidence of protostellar collapse with the BIMA Interferometer at a wavelength of 3 mm. The observations provide a probe of the transition region between the inner envelopes and possible Keplerian disks. The overall goal is to trace the flow of matter during protostellar collapse from the extended envelope to the disk. In particular, the observations reported here will allow us to constrain the mass of disks at the earliest stages of star formation. We are using dust continuum emission to trace the matter. By combining single-dish submillimeter observations with millimeter interferometric observations, we can trace matter on a wide range of scales.

Affiliated with

Also associated with

No associations

Rating

BIMA Observations of B335 and L1527, Two Class 0 Collapsing Protostars does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with BIMA Observations of B335 and L1527, Two Class 0 Collapsing Protostars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and BIMA Observations of B335 and L1527, Two Class 0 Collapsing Protostars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-995985