Radio continuum emission from young stellar objects in L1641

Details Radio continuum emission from young stellar objects in L1641 Radio continuum emission from young stellar objects in L1641

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...362..274m&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 362, Oct. 10, 1990, p. 274-283.

Astronomy and Astrophysics

Astrophysics

27

Continuous Radiation, Early Stars, Orion Nebula, Pre-Main Sequence Stars, Radio Emission, Stellar Radiation, Extragalactic Radio Sources, Herbig-Haro Objects, Stellar Luminosity, Stellar Winds

Scientific paper

The results of a 6 and 20 cm radio continuum survey of young stellar objects in the L1641 region located south of the Orion Nebula are presented. Four are identified as low-luminosity young stellar objects in L1641 and three more as Herbig-Haro or Herbig-Haro-like objects. These objects have bolometric luminosities between 80 and 300 solar, and their 6-20 cm spectral index suggests optically thick, free-free emission. They are characterized by a rising spectrum between 2.2 and 25 microns, have no optical counterparts, and are associated with stellar wind activity. Thus, detectable radio continuum emission may be produced only by the youngest and most luminous objects in L1641.

Affiliated with

Also associated with

No associations

Rating

Radio continuum emission from young stellar objects in L1641 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 emission from young stellar objects in L1641, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radio continuum emission from young stellar objects in L1641 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1302309