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MEL93 - Discovery of Interstellar Water Lines at 437, 439, and 471 GHz: Strong Case for Water Maser Formation behind C-Type Shocks

Short title: Melnick et al. (1993)
Authors: Melnick, Gary J.Menten, Karl M.Phillips, Thomas G.Hunter, Todd
Journal: Astrophysical Journal Letters v.416, p.L37
Bibcode: 1993ApJ...416L..37M
  • Detection table from Melnick et al. (1993)

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    Non-detection table from Melnick et al. (1993)

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    X
    DSS colored
    2MASS colored
    WISE colored
    SDSS color
    IRAC color I1,I2,I4
    GLIMPSE 360
    PACS color (70-160 um)
    SPIRE color (250-500 um)
    NVSS (1.4GHz)
    ATLASGAL 870 um
    ATLASGAL 870 um + Planck
    Bolocam 1.1 mm
    UKIDSS K

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    2MASS K

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