NDLI: Studies of low-mass star formation with the large deployable reflector

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Studies of low-mass star formation with the large deployable reflector

Content Provider	NASA Technical Reports Server (NTRS)
Author	Hollenbach, D. J. Tielens, Alexander G. G. M.
Copyright Year	1984
Description	Estimates are made of the far-infrared and submillimeter continuum and line emission from regions of low mass star formation. The intensity of this emission is compared with the sensitivity of the large deployable reflector (LDR), a large space telescope designed for this wavelength range. The proposed LDR is designed to probe the temperature, density, chemical structure, and the velocity field of the collapsing envelopes of these protostars. The LDR is also designed to study the accretion shocks on the cores and circumstellar disks of low-mass protostars, and to detect shock waves driven by protostellar winds.
File Size	1066153
Page Count	30
File Format	PDF
Alternate Webpage(s)	http://archive.org/details/NASA_NTRS_Archive_19840024258
Archival Resource Key	ark:/13960/t1ng9gr2t
Language	English
Publisher Date	1984-07-01
Access Restriction	Open
Subject Keyword	Astrophysics Stellar Spectra Stellar Winds Molecular Clouds Stellar Evolution Velocity Distribution Protostars Far Infrared Radiation Stellar Envelopes Shock Waves Reflectors Stellar Composition Planets Astronomical Observatories Stellar Temperature Emission Spectra Telescopes Submillimeter Waves Large Deployable Reflector Line Spectra Large Space Structures Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science
Content Type	Text
Resource Type	Technical Report

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