Astronomy and Astrophysics – Astronomy
Scientific paper
Nov 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007apj...669..459b&link_type=abstract
The Astrophysical Journal, Volume 669, Issue 1, pp. 459-463.
Astronomy and Astrophysics
Astronomy
6
Ism: Individual: Alphanumeric: Iras 16547-4247, Ism: Jets And Outflows, Radio Continuum: Stars, Stars: Formation
Scientific paper
Continuum data at 25 and 88 GHz toward the luminous young stellar object IRAS 16547-4247 (G343.126-0.062) have been obtained with the Australia Telescope Compact Array. The triple emission source identified previously at lower frequencies has been detected at 25 GHz. For frequencies between 1.4 and 25 GHz, the flux density of the central continuum source is well fitted with a power-law dependence that is consistent with thermal emission from a jet. The two outer lobes are radio Herbig-Haro objects exhibiting thermal and nonthermal synchrotron emission. At 88 GHz, one unresolved emission source was detected, centered on the radio jet. At this frequency the emission does not arise from the jet but from the dusty molecular envelope within which the jet is embedded.
Brooks Kate J.
Garay Guido
Rodriguez Luis F.
Voronkov Maxim
No associations
LandOfFree
Continuum Observations at 3 and 12 mm of the High-Mass Protostellar Jet IRAS 16547-4247 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 Continuum Observations at 3 and 12 mm of the High-Mass Protostellar Jet IRAS 16547-4247, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Continuum Observations at 3 and 12 mm of the High-Mass Protostellar Jet IRAS 16547-4247 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1696861