2008/01/01 by Kotaro Kohno, K. Kohno, Kazuyuki Muraoka +30
Physics and Astronomy · #Astronomy #Astrophysics #Astrophysics and Cosmic Phenomena #Astrophysics and Star Formation Studies #Bolometer #Detector #Galaxies: Formation, Evolution, Phenomena #Galaxy #Hydrogen line #Luminous infrared galaxy #Millimeter #Optics #Physics #Star formation #Submillimeter Array #Telescope #Tracing #astro-ph
paper · pdf · doi:10.1051/eas:0831013
6 pages, 5 figures, To appear in proceedings of "Far-Infrared and Submillimeter Emission of the Interstellar Medium", EAS Publication Series, Bad Honnef, November 2007, Eds. C. Kramer, S. Aalto, R. Simon. See http://www.nro.nao.ac.jp/~f0212kk/FIR07/kk-ver20.pdf for a version with high resolution figures
openalex publication_date 2008/01/01 · arxiv created 2008/05/13 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
We report our recent progress on extragalactic spectroscopic and continuum observations, including HCN(J=1–0), HCO+(J=1–0), and CN(N=1–0) imaging surveys of local Seyfert and starburst galaxies using the Nobeyama Millimeter Array, high-J CO observations (J=3–2 observations using the Atacama Submillimeter Telescope Experiment (ASTE) and J=2–1 observations with the Submillimeter Array) of galaxies, and λ 1.1 mm continuum observations of high-z violent starburst galaxies using the bolometer camera AzTEC mounted on ASTE.