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Data: H2O

SOB18 - Sun-sized Water Vapor Masers in Cepheus A

  Interferometry data

Short title: Sobolev et al. (2018)
Authors: Sobolev, A. M. Moran, J. M. Gray, M. D. Alakoz, A. Imai, H. Baan, W. A. Tolmachev, A. M. Samodurov, V. A. Ladeyshchikov, D. A.
Journal: The Astrophysical Journal, Volume 856, Issue 1, article id. 60, 9 pp. (2018).
Bibcode: 2018ApJ...856...60S

PDF: SOB18.pdf

Detection table from Sobolev et al. (2018)

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ID Obs. RA Obs. Dec RA offset Dec offset l b Group id # Location Source name Image Descr. Vpeak Fpeak Telescope Detection
(J2000) (J2000) (arcsec) (arcsec) (deg.) (deg.) (km/s) (Jy) Yes/No
1+22 56 17.977+62 01 49109.8709342.114158G109.871+2.114
CepA Image Descr -16.9 .. 0.655 .. 800RA+H2O +CH3OH I +CH3OH II +OH
+22 56 18.017+62 01 51.29080.62.29109.8712772.1147001HW3diiiCepA0.6580
+22 56 17.3303+62 01 50.6408-9.71.64109.8699872.1151122HW3diiCepA-9.7800
+22 56 16.9903+62 01 49.0508-14.80.05109.8691972.1149983HW2CepA-14.855
+22 56 16.897+62 01 49.0108-16.20.01109.8690272.1150664HW2CepA-16.2130
+22 56 16.8503+62 01 49.0008-16.90 mas109.8689442.1151035HW2CepA-16.9152
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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

    Tip: Use "Box select" or "Lasso select" to display colour-selected sources in Aladin all-sky view

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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 SOB18

    Tip: Use "Box select" or "Lasso select" to display velocity-selected sources in Aladin all-sky view

    Tip: Click on some source to look at the different surveys. You must select some surveys in previous page at "View images"

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

  • Distribution of sources from SOB18 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
    2MASS K