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Wednesday, May 6, 2020 | History

3 edition of Studies of low-mass star formation with the large deployable reflector found in the catalog.

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

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

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  • 30 Currently reading

Published by National Aeronautics and Space Administration, Ames Research Center in Moffett Field, Calif .
Written in English

    Subjects:
  • Stars -- Masses

  • Edition Notes

    StatementA.G.G.M. Tielens, D.J. Hollenbach
    SeriesNASA technical memorandum -- 85960
    ContributionsHollenbach, David J, Ames Research Center
    The Physical Object
    FormatMicroform
    Pagination1 v.
    ID Numbers
    Open LibraryOL17977486M

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    Applications of long-baseline systems to studying asteroids, comets, star formation, and galactic nuclei are discussed, noting the large advantages available in visible wavelength studies if the instrumentation was space-based. Mizoram State Data Center Request for Proposal (Vol II) For Setting up of State Data Center in Secretariat Building, Annex – 1, Treasury Square, Aizawl Ref No D/14/MSeGS Date: 17th August, State Implementing Agency MSeGS MIZORAM STATE eGOVERNANCE SOCIETY. Govt. Of Mizoram. Secretariat Building, Annex-1, Treasury Square.

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Studies of low-mass star formation with the large deployable reflector Download PDF EPUB FB2

Get this from a library. Studies of low-mass star formation with the large deployable reflector. [A G G M Tielens; David J Hollenbach; Ames Research Center.]. The JWST has an expected mass about half of Hubble Space Telescope's, but its primary mirror (a meter diameter, foot gold-coated beryllium reflector) will have a collecting area about five times as large (25 m 2 or sq ft vs.

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