Compact Extragalactic Star Formation: Peering Through the Dust at Centimeter Wavelengths

Details Compact Extragalactic Star Formation: Peering Through the Dust at Centimeter Wavelengths Compact Extragalactic Star Formation: Peering Through the Dust at Centimeter Wavelengths

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005assl..329..127u&link_type=abstract

Starbursts: From 30 Doradus to Lyman Break Galaxies, Held in Cambridge, UK, 6-10 September 2004. Edited by R. de Grijs and R.M.

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

We summarize results of arcsecond and milliarcsecond-resolution radio imaging of starbursts. Thermal radio emission from young super star clusters (SSCs) indicates that they are powered by the equivalent of hundreds to thousands of O7 stars. Milliarcsecond imaging of Arp 299 reveals individual young supernovae that are factors of ˜ 100 more powerful than Cas A, and that may show the locations of older SSCs in which the most massive stars already have gone supernova.

Affiliated with

Also associated with

No associations

Rating

Compact Extragalactic Star Formation: Peering Through the Dust at Centimeter Wavelengths 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 Compact Extragalactic Star Formation: Peering Through the Dust at Centimeter Wavelengths, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Compact Extragalactic Star Formation: Peering Through the Dust at Centimeter Wavelengths will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1701435