(Sub)mm Interferometry Applications in Star Formation Research

2006/11/22 by H. Beuther, Henrik Beuther
Chemistry · Physics and Astronomy · #Accretion (finance) #Accretion disc #Angular resolution (graph drawing) #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Computer science #Galaxies: Formation, Evolution, Phenomena #Geology #High resolution #Interferometry #Molecular Spectroscopy and Structure #Optics #Physics #Remote sensing #Resolution (logic) #Star (game theory) #Star formation #Stars #Wavelength #astro-ph

paper · pdf · doi:10.1007/978-3-540-68032-1_10

published as Lect.NotesPhys.742:219-239,2008 · 20 pages, 7 figures, in proceedings to "2nd European School on Jets from Young Star: High Angular Resolution Observations". A high-resolution version of the paper can be found at http://www.mpia.de/homes/beuther/papers.html

arxiv created 2006/11/22 · openalex publication_date 2007/10/30 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

This contribution gives an overview about various applications of (sub)mm interferometry in star formation research. The topics covered are molecular outflows, accretion disks, fragmentation and chemical properties of low- and high-mass star-forming regions. A short outlook on the capabilities of ALMA is given as well.

Citations

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