2008/05/05 by R. Paladino, M. Murgia, A. Tarchi +2
Physics and Astronomy · #Astronomy #Astrophysics #Astrophysics and Cosmic Phenomena #Galaxies: Formation, Evolution, Phenomena #Galaxy #Infrared #Interferometry #Physics #Plateau de Bure Interferometer #Radio Astronomy Observations and Technology #Radio galaxy #Spiral galaxy #Star formation #astro-ph
paper · pdf · doi:10.1051/0004-6361:20079135
17 pages, 17 figures (low resolution). Accepted for publication in A&A. Some language and reference changes done. High resolution version of the paper is available at: http://erg.ca.astro.it/~rpaladin/PAPER/NGC3627/AA9135.ps
arxiv created 2008/05/05 · openalex publication_date 2008/05/06 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Aims. We present new radio observations of two regions of the spiral galaxy NGC 3627, including new radio continuum observations at 1.4 GHz with the Very Large Array, and also new observations in the CO line, taken with the Plateau de Bure interferometer. Comparing these observations with archival Spitzer and Hα data we study the correlation of the radio continuum (RC), infrared-8 , and CO emissions at a spatial resolution of 100 pc.