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GOR17 - Survey of Water and Ammonia in Nearby Galaxies (SWAN): Resolved Ammonia Thermometry, and Water and Methanol Masers in the Nuclear Starburst of NGC 253

  Interferometry data

Short title: Gorski et al. (2017)
Authors: Gorski, Mark Ott, Jürgen Rand, Richard Meier, David S. Momjian, Emmanuel Schinnerer, Eva
Journal: The Astrophysical Journal, Volume 842, Issue 2, article id. 124, 21 pp. (2017).
Bibcode: 2017ApJ...842..124G

Detection table from Gorski et al. (2017)

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ID Obs. RA Obs. Dec RA offset Dec offset l b Group id # Maser spot Source name Image Descr. Line Vpeak Ta ∫Ta dv Telescope Beam Detection Class Dist. (parallax) Date
(J2000) (J2000) (mas) (mas) (deg.) (deg.) CH3OH (class I) (km/s) (K) (K*km/s) (arcsec) Yes/No (kpc)
1+00 47 34.1-25 17 11.797.483003-87.964082G97.224-87.965
NGC 253 Image Descr 36 GHz (I); 165.9 .. 331.60.026 .. 0.0561.38 .. 3.59NRAOVLA2 x 1+CH3OH I GALAXY2013 May
+00 47 34.1-25 17 11.70 mas0 mas97.483003-87.9640821M1NGC 253202.0 (0.3)0.026 (0.005)1.38 (0.07)
+00 47 33.9-25 17 10.8-2998.8 mas898.8 mas97.466765-87.9635362M2NGC 253195.4 (0.8)0.040 (0.006)1.41 (0.07)
+00 47 33.7-25 17 13.1-5998.8 mas-1401.2 mas97.439941-87.9637963M3NGC 253165.9 (1.7)0.039 (0.008)3.59 (0.14)
+00 47 31.9-25 17 25.7-32998.8 mas-14001.2 mas97.225298-87.9640804M4NGC 253294.1 (2.6)0.035 (0.005)3.09 (0.18)
+00 47 32-25 17 28.9-31498.8 mas-17201.2 mas97.224204-87.9650445M5NGC 253294.3 (3.0)0.056 (0.005)2.19 (0.89)
+00 47 32-25 17 28.9-31498.8 mas-17201.2 mas97.224204-87.9650446M5NGC 253331.6 (10.2)0.041 (0.005)2.33 (0.96)
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  • Distribution of sources in all sky (l,b)

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  • Distribution of sources in all sky using Aladin

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  • Distribution of sources in IRAS color-color diagram

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    Original color diagram is taken form van der Veen & Habing (1987)

    Type Description
    I Oxygen-rich non-variable stars without circumstellar shells
    II Variable stars with "young" O-rich circumstellar shells
    IIIa Variable stars with more evolved O-rich circumstellar shells
    IIIb Variable stars with thick O-rich circumstellar shells
    IV Variable stars with very thick O-rich circumstellar shells
    V Planetary nebulae and non- variable stars with very cool circumstellar shells
    VIa Variable stars with relatively cold dust at large distances; a significant part of the stars is carbon-rich
    VIb Variable stars with relatively hot dust close to the star and relatively cold dust at large distances; Some of the objects have proven to be O-rich
    VII Variable stars with more evolved C-rich circumstellar shells
    VIII Different sort of objects

  • Distribution of the detection velocities versus galactic longitude from GOR17

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    Longitude-Velocity Map is taken form Dame, Hartmann & Thaddeus (2001)

  • Distribution of sources from GOR17 in (l,b) histograms



    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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