Display data from paper

Select data type: CH3OH_I

KAL10B - VLA observations of class I methanol masers in the region of low-mass star formation L1157

  Interferometry data

Short title: Kalenskii et al. (2010B)
Authors: Kalenskii, S. V. Kurtz, S. Slysh, V. I. Hofner, P. Walmsley, C. M. Johansson, L. E. B. Bergman, P.
Journal: Astronomy Reports, Volume 54, Issue 10, pp.932-939
Bibcode: 2010ARep...54..932K

PDF: KAL10B.pdf

Detection table from Kalenskii et al. (2010B)

Export table to csv

Hide / Show individual components

ID Obs. RA Obs. Dec RA offset Dec offset l b Group id # Location 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+20 39 09+68 01 42102.64889115.787184G102.641+15.784
L1157 Image 44 GHz (I)
-0.5 .. 1.7 .. .. NRAOVLA1.87 x 1.45+H2O +CH3OH I -CH3OH II March 17, 2007
+20 39 10.033+68 01 42.215.4950.2012102.64988515.7858881M1aL11570.80.4000.2008.000
+20 39 10.107+68 01 42.4216.6050.4212102.65000515.7858272M1bL1157-0.50.6000.400165.000
+20 39 9.465+68 01 15.596.975-26.4088102.64303115.7824363M2L11571.71.9000.700129.000
×
×
  • 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 KAL10B

    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 KAL10B 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