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Source: The Open Library

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1Cometary atmospheres

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“Cometary atmospheres” Metadata:

  • Title: Cometary atmospheres
  • Author:
  • Language: English
  • Publisher: ➤  For sale by the Clearinghouse for Federal Scientific and Technical Information - National Aeronautics and Space Administration
  • Publish Date:
  • Publish Location: ➤  [Washington, DC - [Springfield, Va - [Washington, DC] - Springfield, Va

“Cometary atmospheres” Subjects and Themes:

Edition Identifiers:

Access and General Info:

  • First Year Published: 1985
  • Is Full Text Available: No
  • Is The Book Public: No
  • Access Status: No_ebook

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    2Hot absorbers and the X-ray spectra of BL Lac objects

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    “Hot absorbers and the X-ray spectra of BL Lac objects” Metadata:

    • Title: ➤  Hot absorbers and the X-ray spectra of BL Lac objects
    • Author:
    • Language: English
    • Publisher: ➤  National Technical Information Service, distributor - Space Telescope Science Institute - National Aeronautics and Space Administration
    • Publish Date:
    • Publish Location: ➤  Springfield, Va - [Washington, DC - Baltimore, MD

    “Hot absorbers and the X-ray spectra of BL Lac objects” Subjects and Themes:

    Edition Identifiers:

    Access and General Info:

    • First Year Published: 1994
    • Is Full Text Available: No
    • Is The Book Public: No
    • Access Status: No_ebook

    Online Access

    Downloads Are Not Available:

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      3The effects of pure density evolution on the brightness distribution of cosmological gamma-ray bursts

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      “The effects of pure density evolution on the brightness distribution of cosmological gamma-ray bursts” Metadata:

      • Title: ➤  The effects of pure density evolution on the brightness distribution of cosmological gamma-ray bursts
      • Author:
      • Language: English
      • Publisher: ➤  National Technical Information Service, distributor - National Aeronautics and Space Administration
      • Publish Date:
      • Publish Location: ➤  Springfield, Va - [Washington, D.C

      “The effects of pure density evolution on the brightness distribution of cosmological gamma-ray bursts” Subjects and Themes:

      Edition Identifiers:

      Access and General Info:

      • First Year Published: 1995
      • Is Full Text Available: No
      • Is The Book Public: No
      • Access Status: No_ebook

      Online Access

      Downloads Are Not Available:

      The book is not public therefore the download links will not allow the download of the entire book, however, borrowing the book online is available.

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        4The mass and dynamics of cD clusters with cooling flows

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        “The mass and dynamics of cD clusters with cooling flows” Metadata:

        • Title: ➤  The mass and dynamics of cD clusters with cooling flows
        • Author:
        • Language: English
        • Publisher: ➤  National Technical Information Service, distributor - National Aeronautics and Space Administration
        • Publish Date:
        • Publish Location: ➤  Springfield, Va - [Washington, DC

        “The mass and dynamics of cD clusters with cooling flows” Subjects and Themes:

        Edition Identifiers:

        Access and General Info:

        • First Year Published: 1994
        • Is Full Text Available: No
        • Is The Book Public: No
        • Access Status: No_ebook

        Online Access

        Downloads Are Not Available:

        The book is not public therefore the download links will not allow the download of the entire book, however, borrowing the book online is available.

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          5A study of cooling flows in poor clusters of galaxies

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          “A study of cooling flows in poor clusters of galaxies” Metadata:

          • Title: ➤  A study of cooling flows in poor clusters of galaxies
          • Author:
          • Language: English
          • Publisher: ➤  National Technical Information Service, distributor - National Aeronautics and Space Administration
          • Publish Date:
          • Publish Location: ➤  Springfield, Va - [Washington, D.C

          “A study of cooling flows in poor clusters of galaxies” Subjects and Themes:

          Edition Identifiers:

          Access and General Info:

          • First Year Published: 1995
          • Is Full Text Available: No
          • Is The Book Public: No
          • Access Status: No_ebook

          Online Access

          Downloads Are Not Available:

          The book is not public therefore the download links will not allow the download of the entire book, however, borrowing the book online is available.

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            Wiki

            Source: Wikipedia

            Wikipedia Results

            Search Results from Wikipedia

            Very-long-baseline interferometry

            visibility depends on the symmetry of the source brightness distribution. Any brightness distribution can be written as the sum of a symmetric component

            Van Cittert–Zernike theorem

            object, a radio astronomer can thereby reconstruct the source's brightness distribution and make a two-dimensional map of the source's appearance. Consider

            List of brightest stars

            arranged by their apparent magnitude – their brightness as observed from Earth. It includes all stars brighter than magnitude +2.50 in visible light, measured

            Sky brightness

            significantly. The total brightness of all the stars was first measured by Burns in 1899, with a calculated result that the total brightness reaching earth was

            Image histogram

            particular brightness or tonal value (horizontal axis). Algorithms in the digital editor allow the user to visually adjust the brightness value of each

            José Luis Sérsic

            is named in his honour. J. L. Sérsic (1963), Influence of the atmospheric and instrumental dispersion on the brightness distribution in a galaxy v t e

            Altair

            Nordgren, Tyler E.; Hutter, Donald J. (2004). "Asymmetric Surface Brightness Distribution of Altair Observed with the Navy Prototype Optical Interferometer"

            AstroSat

            with a two dimensional coded mask, for imaging purposes. The sky brightness distribution will be obtained by applying a deconvolution procedure to the shadow

            Color histogram

            expressed as “three luminance histograms”, each of which shows the brightness distribution of each individual red/green/blue color channel. A color histogram

            WD J2147–4035

            0.55 ±0.03 Megagauss. The magnetism can lead to inhomogeneous brightness distribution and the TESS light curve shows that the white dwarf has a rotation