The Interaction Between the Supernova Remnant W41 and the Filamentary Infrared Dark Cloud G23.33-0.30
| Autor: | David Allingham, Ian W. Stephens, J. Scott Whitaker, Andrés E. Guzmán, Nicholas Killerby-Smith, Taylor Hogge, Patricio Sanhueza, Kathleen E. Kraemer, James M. Jackson |
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| Jazyk: | angličtina |
| Rok vydání: | 2019 |
| Předmět: |
Physics
010504 meteorology & atmospheric sciences Molecular cloud FOS: Physical sciences Velocity dispersion Astronomy and Astrophysics Astrophysics 01 natural sciences Astrophysics - Astrophysics of Galaxies Virial theorem Space and Planetary Science Astrophysics of Galaxies (astro-ph.GA) 0103 physical sciences Infrared dark cloud Continuum (set theory) Supernova remnant 010303 astronomy & astrophysics Energy (signal processing) 0105 earth and related environmental sciences Line (formation) |
| Popis: | G23.33-0.30 is a 600 $M_{\odot}$ infrared dark molecular filament that exhibits large NH$_3$ velocity dispersions ($\sigma \sim 8 \ \rm{km \ s^{-1}}$) and bright, narrow NH$_3$(3,3) line emission. We have probed G23.33-0.30 at the $ |
| Databáze: | OpenAIRE |
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