Radio Continuum Maps of Deeply Embedded Protostars: Thermal Jets, Multiplicity, and Variability

Details Radio Continuum Maps of Deeply Embedded Protostars: Thermal Jets, Multiplicity, and Variability Radio Continuum Maps of Deeply Embedded Protostars: Thermal Jets, Multiplicity, and Variability

Aug 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aj....124.1045r&link_type=abstract

The Astronomical Journal, Volume 124, Issue 2, pp. 1045-1053.

Astronomy and Astrophysics

Astronomy

63

Stars: Binaries: General, Ism: Jets And Outflows, Radio Continuum, Stars: Formation, Stars: Pre-Main-Sequence

Scientific paper

We have carried out a deep, 3.6 cm radio continuum survey of young outflow sources using the Very Large Array in its A configuration providing subarcsecond resolution. The seven regions observed are L1448-N, IRAS 2 and 4 in NGC 1333, L1551-NE, SSV 63 in L1630, HH 124 IRS in NGC 2264, and B335 IRS. The first three of these objects are known from submillimeter observations to be multiple sources, and we detect almost all known submillimeter components at 3.6 cm. The L1551-NE source is confirmed to be a subarcsecond binary. We find a third radio source in the SSV 63 system, which drives the multiple HH 24 jets. HH 124 IRS is embedded in a cometary cloud, where we detect a small cluster of six time-variable radio continuum sources. Six of the observed sources are resolved into compact thermal radio jets.

Affiliated with

Also associated with

No associations

Rating

Radio Continuum Maps of Deeply Embedded Protostars: Thermal Jets, Multiplicity, and Variability 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 Radio Continuum Maps of Deeply Embedded Protostars: Thermal Jets, Multiplicity, and Variability, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radio Continuum Maps of Deeply Embedded Protostars: Thermal Jets, Multiplicity, and Variability will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1674700