The stellar populations within the OPH cloud cores

Details The stellar populations within the OPH cloud cores The stellar populations within the OPH cloud cores

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.217..223s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 217, no. 1-2, p. 223-224

Astronomy and Astrophysics

Astronomy

1

Accretion Disks, Infrared Stars, Molecular Clouds, Radio Sources (Astronomy), Star Formation, Stellar Activity, Stellar Color, Stellar Envelopes, Stellar Magnitude, Cores, Infrared Astronomy, Ionization, Populations, Radio Astronomy, Stellar Physics, Stellar Winds, Synchrotron Radiation, Very Large Array (Vla)

Scientific paper

We have obtained infrared colors and limiting magnitudes from 1.25-4.8 micrometers for a sample of 26 of the cm continuum radio sources located in the core of the rho Oph molecular cloud. Their colors demonstrate that the majority of the sources appear to be heavily reddened objects surrounded by circumstellar accretion disks. In these cases the radio emission most likely diagnoses accretion driven energetic outflow phenomena: either ionized winds or possibly synchrotron emission from shocked gas associated with stellar jets.

Affiliated with

Also associated with

No associations

Rating

The stellar populations within the OPH cloud cores 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 The stellar populations within the OPH cloud cores, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The stellar populations within the OPH cloud cores will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1252780