Display data from paper

Select data type: OH

LEW01 - The Approaching Death of the OH/IR star IRAS 18455+0448

Short title: Lewis et al. (2001)
Authors: Lewis, B. M. Oppenheimer, B. D. Daubar, I. J.
Journal: The Astrophysical Journal, Volume 548, Issue 1, pp. L77-L80.
Bibcode: 2001ApJ...548L..77L

Detection table from Lewis et al. (2001)

Export table to csv

Hide / Show individual components

ID Obs. RA Obs. Dec l b Group id Source name Frequency Vrange Vpeak Fpeak List Detection Ref.
(J2000) (J2000) (deg.) (deg.) (MHz) (km/s) (km/s) (Jy) Yes/No
118 48 2.1+04 51 2936.87222.9683G36.873+2.968
IRAS 18455+0448161227.827.80.040ENG15+H2O +OH LEW01
18 48 2.1+04 51 2936.87222.9683G36.873+2.968
IRAS 18455+0448166512.527.90.454ENG15+H2O +OH LEW01
18 48 2.1+04 51 2936.87222.9683G36.873+2.968
IRAS 18455+0448166712.627.70.733ENG15+H2O +OH LEW01
×
×
  • 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 LEW01

    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 LEW01 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