EXTENDED HCN AND HCO+EMISSION IN THE STARBURST GALAXY M82
Authors:
- P. SalasPSP. Salas
- A. KepleyAKA. Kepley
- 8 December 2014
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 797 (2)
Abstract
No abstract availableAll Related Versions
This publication has 48 references indexed in Scilit:
- Astropy: A community Python package for astronomyAstronomy & Astrophysics, 2013
- Suppression of star formation in the galaxy NGC 253 by a starburst-driven molecular windNature, 2013
- Spectroscopic FIR mapping of the disk and galactic wind of M 82 withHerschel-PACSAstronomy & Astrophysics, 2013
- Aλ= 1.3 mm and 2 mm molecular line survey towards M 82Astronomy & Astrophysics, 2011
- CS, HC3N, and CH3CCH multi-line analyses toward starburst galaxiesAstronomy & Astrophysics, 2010
- THE ACS NEARBY GALAXY SURVEY TREASURYThe Astrophysical Journal Supplement Series, 2009
- Structure and kinematics within the Starburst nucleus of M82: Searching for a barThe Astrophysical Journal, 1995
- High-resolution X-ray imaging of the Starburst Galaxy M82The Astrophysical Journal, 1995
- H II regions in M82 - High-resolution millimeter continuum observationsThe Astrophysical Journal, 1991
- Infrared imaging and polarimetry of M82 - Evidence for a ring of warm dustThe Astronomical Journal, 1989