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

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

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984stin...8432328h&link_type=abstract

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Astronomy and Astrophysics

Astronomy

Astronomical Observatories, Emission Spectra, Far Infrared Radiation, Large Deployable Reflector, Large Space Structures, Line Spectra, Molecular Clouds, Protostars, Reflectors, Shock Waves, Stellar Envelopes, Stellar Evolution, Stellar Spectra, Submillimeter Waves, Telescopes, Planets, Stellar Composition, Stellar Temperature, Stellar Winds, Velocity Distribution

Scientific paper

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.

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