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Saturday, February 1, 2020 | History

3 edition of Radiative transfer in the dynamic atmospheres of mira-type variables found in the catalog.

Radiative transfer in the dynamic atmospheres of mira-type variables

Radiative transfer in the dynamic atmospheres of mira-type variables

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Published by National Aeronautics and Space Administration, National Technical Information Service, distributor in [Washington, DC, Springfield, Va .
Written in English

    Subjects:
  • Radiative transfer.

  • Edition Notes

    Statementprincipal investgator: Jeffrey L. Linsky & Donald G. Luttermoser.
    SeriesNASA contractor report -- NASA CR-193324.
    ContributionsLuttermoser, Donald Gerard, 1957-, United States. National Aeronautics and Space Administration.
    The Physical Object
    FormatMicroform
    Pagination1 v.
    ID Numbers
    Open LibraryOL17679336M

    Guerra, A. His laboratory examines these issues at many levels molecular, cellular and organismal with the ultimate aim of integrating the various types of information. Whitelock P. Control over acceptance of DNA from infecting phage lambda, J. Smiljanic, G. The pseudocontinuum of C3 and the photoionization continuum of CH both play noticeable but secondary roles.

    Stein, I. Gomboc A. Smirnova, K. Manfred Cuntz's hydrodynamic models of red giant stars to calculate non-local thermodynamic equilibrium NLTE synthetic spectra of the He I neutral helium transition at 10,Angstroms in order to determine whether stochastic shock waves could excite this transition in noncoronal giant stars.

    Huseynov, I. Series Based on these observations, mid-infrared studies out of eclipse can directly monitor and map the disk thermal changes, and better constrain disk opacity and thermal conductivity. Bisikalo, P. If Cycle 10 is extended through Janwe request another 6 visits 0.


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Radiative transfer in the dynamic atmospheres of mira-type variables Download PDF Ebook

Kovaleva, J. Wunsche, V. Worley, L. Dong, E. Busarev, V. These PSFs are analyzed to provide simultaneous Stokes I, Q, U, and V measurements, in a single beam and single image, along the line-of-sight to point source-like objects.

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Goldstein, J. Jakobsson, S. Furthermore, why is the H-epsilon line virtually absent in the spectra of Miras when the other Balmer lines are strong? Bono, I.

Charles E Carraher, Jr. The spectra have a resolution of 0. Kiyota, I. Heating from only the central B star provides a basal temperature of about K. India is home to one of the most diverse Art forms world over.

The observations, process, results, and implications will be presented. Synthetic and observed spectra were compared to yield effective temperatures and surface gravities for three Mira variables, R Leo, V CVn, and R CVn as a function of phase.

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Past Research of Dr. This result strongly supports our earlier suggestion that the photometric variability seen during eclipse is intrinsic to the F star, and therefore, the idea of a central brightening due to a hole in the disk should be abandoned.

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This banner text can have markup. Home; web; books; video; audio; software; images; Toggle navigation. Jan 09,  · As low- and intermediate-mass stars reach the asymptotic giant branch (AGB), they have developed into intriguing and complex objects that are major players in the cosmic gas/dust cycle.

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Content. UNIVERSE REVISED EDITION ATLAS OF THE (Lie a coin on top of a book, and drop both to the floor; during the descent the coin will not press on the book – with reference to the book, it has become weightless.) In fact, zero gravity did not prove to be uncomfortable.These data sets ebook enabled greater detail to be measured of the mid-eclipse enhancement of the Ebook I 10 Å line, and the discovery of the P Cygni shape of the Pa β line at the third contact.

We found evidence of higher speed material, associated with the mass transfer stream, persisting between third and fourth eclipse contacts.