Display data from paper

Select data type: CH3OH_II

SAN17 - Planar infall of CH3OH gas around Cepheus A HW2

Short title: Sanna et al. (2017)
Authors: Sanna, A.Moscadelli, L.Surcis, G.van Langevelde, H. J.Torstensson, K. J. E.Sobolev, A. M.
Journal: Astronomy & Astrophysics, Volume 603, id.A94, 9 pp.
Bibcode: 2017A&A...603A..94S

Detection table from Sanna et al. (2017)

Export table to csv

Hide / Show individual components

ID Obs. RA Obs. Dec l b Group id Source name Image Line Vpeak Telescope RMS Beam Detection Class Dist. (parallax) Date
(J2000) (J2000) (deg.) (deg.) CH3OH (class II) (km/s) (Jy) (arcsec) Yes/No (kpc)
122 56 17.9+62 01 49.5109.87092.1143G109.871+2.114
Cepheus A HW2 Image 6.6 GHz (II); -1.73EVN6.0004.5+H2O +CH3OH I +CH3OH II +OH SFR2013-2015
×
×
  • Distribution of sources in all sky (l,b)

    0

  • Distribution of sources in all sky using Aladin

    Tip: Click on some source to get more informaiton


  • 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

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

    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 SAN17

    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 SAN17 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

    Download UKIDSS K FITS
    2MASS K

    Download 2MASS K FITS