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Astrochemistry / Star formation / Stellar astronomy / Radio astronomy / Molecular cloud / Astrophysical maser / H II region / Interstellar medium / Young stellar object / Astronomy / Space / Nebulae


HOT MOLECULAR CORES AND THE EARLIEST PHASES OF HIGH-MASS STAR FORMATION STAN KURTZ Universidad Nacional Auto´noma de Me´xico RICCARDO CESARONI Osservatorio Astrofisico di Arcetri
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Document Date: 2007-04-05 13:30:20

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Company

HOT MOLECULAR CORES 305 C. Solutions / Hillenbrand / /

Facility

Washburn Observatory PETER HOFNER University of Puerto Rico / noma de Me´xico RICCARDO CESARONI Osservatorio Astrofisico di Arcetri ED CHURCHWELL University of Wisconsin / Arecibo Observatory / /

IndustryTerm

gas clumps / physical and chemical studies / ionized gas component / neutral gas / gravitational energy / ionized gas / molecular gas component / molecular gas / circumstellar molecular gas / dense gas / /

Organization

University of Puerto Rico / University of Wisconsin / MOLECULAR CORES AND THE EARLIEST PHASES OF HIGH-MASS STAR FORMATION STAN KURTZ Universidad Nacional Auto´noma de Me´xico RICCARDO CESARONI Osservatorio Astrofisico / /

Person

C. MALCOLM WALMSLEY / Mundy / /

Position

Hunter / /

ProvinceOrState

Wisconsin / Alabama / /

Technology

recombination / /

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