Display data from paper

Select data type: H2O

SUA09 - Water maser detections in southern candidate post-AGB stars and planetary nebulae

Short title: Suarez et al. (2009)
Authors: Suarez, O. Gomez, J. F. Miranda, L. F. Torrelles, J. M. Gómez, Y. Anglada, G. Morata, O.
Journal: Astronomy and Astrophysics, Volume 505, Issue 1, 2009, pp.217-225
Bibcode: 2009A&A...505..217S

Detection table from Suarez et al. (2009)

Export table to csv

Hide / Show individual components

ID Obs. RA Obs. Dec l b Group id Source name Vrange Vpeak Fpeak ∫F dv RMS Detection
(J2000) (J2000) (deg.) (deg.) (km/s) (km/s) (Jy) (Jy*km/s) (Jy) Yes/No
112 43 31.5-62 36 14302.02180.2539G302.022+0.254
IRAS 12405-6219-23.60.9411.10.120+H2O -CH3OH II
213 53 34.5-61 20 52310.31040.6306G310.310+0.631
IRAS 13500-610639.90.88.90.150+H2O -CH3OH II -OH
13 53 34.5-61 20 52310.31040.6306G310.310+0.631
IRAS 13500-610640.01.66.70.230+H2O -CH3OH II -OH
315 14 18.5-58 05 20320.9066-0.2928G320.906-0.293
IRAS 15103-575480.0-35.860.31327.60.240+H2O -OH
15 14 18.5-58 05 20320.9066-0.2928G320.906-0.293
IRAS 15103-575480.0-35.836.7704.60.600+H2O -OH
416 37 6.1-48 13 42336.6430-0.6944G336.644-0.695
IRAS 16333-4807-42.21.8260.200+H2O +OH
×
×
  • 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 SUA09

    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 SUA09 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