Display data from paper

Select data type: CH3OH_I, CH3OH_II

VOR05 - The 6.7- and 25-GHz methanol masers in OMC-1

  Interferometry data

Short title: Voronkov et al. (2005)
Authors: Voronkov, M. A. Sobolev, A. M. Ellingsen, S. P. Ostrovskii, A. B.
Journal: Monthly Notices of the Royal Astronomical Society, Volume 362, Issue 3, pp. 995-1005.
Bibcode: 2005MNRAS.362..995V

Detection table from Voronkov et al. (2005)

Export table to csv

Hide / Show individual components

ID Obs. RA Obs. Dec RA offset Dec offset l b Group id # Source name Image Line Vpeak Fpeak ∫F dv Major Minor PA Telescope Beam Detection Date
(J2000) (J2000) (arcsec) (arcsec) (deg.) (deg.) CH3OH (class I) (km/s) (Jy) (Jy*km/s) (arcsec) (arcsec) (deg.) (arcsec) Yes/No
1+05 35 15-05 23 42.53209.012979-19.391939G208.993-19.385
OMC-1 Image 24.959 GHz (I)
7.34 .. 9.9214 .. 89 .. ATCA120+H2O +CH3OH I +CH3OH II +OH +SiO 2003 June 9-10
+05 35 14.87-05 22 44-1.9558.5292208.997349-19.3850651OMC-17.3435 (2)29.60018.600-63.000
+05 35 14.83-05 22 42.8-2.5559.7292208.996954-19.3850632OMC-17.5848 (2)30.40018.400-64.000
+05 35 14.33-05 22 36.5-10.0566.0292208.994305-19.3861213OMC-17.9568 (5)38.10018.900-57.000
+05 35 14.02-05 22 30.9-14.771.6292208.992217-19.3865644OMC-18.2889 (4)40.00019.300-53.000
+05 35 14.02-05 22 31.8-14.770.7292208.992454-19.3866775OMC-18.7545 (1)35.60020.500-50.000
+05 35 14.19-05 22 14-12.1588.5292208.988117-19.3838116OMC-19.9214 (1)29.90020.700-60.000
×
×
  • Distribution of sources in all sky (l,b)

    Save as PNG, Save as EPS

  • 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 VOR05

    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 VOR05 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