High Resolution 18 Micron Imaging of Hot Molecular Cores
| dc.creator | De Buizer, James M. | |
| dc.date | 2002-07-16 | |
| dc.date.accessioned | 2026-07-07T02:04:20Z | |
| dc.date.available | 2026-07-07T02:04:20Z | |
| dc.description | 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. | |
| dc.description | 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) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0207336 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0207336 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/4712 | |
| dc.subject | Astrophysics | |
| dc.title | High Resolution 18 Micron Imaging of Hot Molecular Cores | |
| dc.type | text |