arXiv Analytics

Sign in

arXiv:astro-ph/0207336AbstractReferencesReviewsResources

High Resolution 18 Micron Imaging of Hot Molecular Cores

James M. De Buizer

Published 2002-07-16Version 1

I present the latest results from a search for hot molecular cores at mid-infrared wavelengths from the largest optical telescopes available at the present time. Three well-observed hot molecular cores were imaged, G29.96-0.02, G19.61-0.23, and G34.26+0.15. Even though mid-infrared sources have been claimed to be detected previously at the hot molecular core locations of both G19.61-0.23 and G34.26+0.15, only the hot molecular core in G29.96-0.02 resulted in a detection. New upper limits on mid-infrared emission are given for the hot molecular cores that were not detected.

Comments: 7 pages, 5 figures, to appear in 'Galactic Star Formation Across the Stellar Mass Spectrum', eds. J.M. De Buizer & N.S. van der Bliek (ASP coference Series, 2002)
Categories: astro-ph
Related articles: Most relevant | Search more
arXiv:astro-ph/0403454 (Published 2004-03-18)
R=100,000 Mid-IR Spectroscopy of UCHII Regions: High Resolution is Worth it!
arXiv:astro-ph/9309053 (Published 1993-09-30)
The metal systems in Q0000--2619 at high resolution
arXiv:0811.0316 [astro-ph] (Published 2008-11-03)
Science with the World Space Observatory - Ultraviolet