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FRA94 - Stellar OH masers toward globular clusters.

Short title: Frail & Beasley (1994)
Authors: Frail, D. A. Beasley, A. J.
Journal: Astronomy and Astrophysics, Vol. 290, p.796-802 (1994)
Bibcode: 1994A&A...290..796F

Detection table from Frail & Beasley (1994)

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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
116 32 24.7-13 12 033.227222.9443G3.227+22.945
IRAS 16296-130516127.0-33.00.150ENG15+OH +SiO FRA94
217 32 49.1-33 24 05354.7632-0.0636G354.762-0.062
IRAS 17295-3321161227.5-13.02.400ENG15+OH +SiO FRA94
317 47 28-33 03 56356.6744-2.4811G356.674-2.481
Djorg 1161229.5-106.51.400ENG15+OH FRA94
418 38 10.3-23 43 1510.2400-7.8335G10.240-7.834
IRAS 18351-2345161212.0-33.00.200ENG15+OH -SiO FRA94
517 35 2.1-33 33 30354.8825-0.5370G354.884-0.538
IRAS 17317-3331161229.5-5.52.200ENG15+H2O +OH +SiO FRA94
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Non-detection table from Frail & Beasley (1994)

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ID Obs. RA Obs. Dec l b Group id Source name Fpeak List Detection Ref.
(J2000) (J2000) (deg.) (deg.) (Jy) Yes/No
118 25 30.1-24 53 437.8752-5.7845G7.875-5.784
IRAS 18224-24550.200ENG15-OH FRA94
218 31 18.5-25 34 067.8708-7.2601G7.871-7.260
IRAS 18282-25360.200ENG15-OH +SiO FRA94
318 37 12.7-23 55 189.9601-7.7256G9.960-7.726
IRAS 18341-23570.200ENG15-OH +SiO FRA94
417 47 28-33 03 56356.6744-2.4811G356.674-2.481
Djorg 10.200ENG15+OH FRA94
518 38 10.3-23 43 1510.2400-7.8335G10.240-7.834
IRAS 18351-23450.200ENG15+OH -SiO FRA94
617 35 2.1-33 33 30354.8825-0.5370G354.884-0.538
IRAS 17317-33310.200ENG15+H2O +OH +SiO FRA94
717 32 49.1-33 24 05354.7632-0.0636G354.762-0.062
IRAS 17295-33210.200ENG15+OH +SiO FRA94
816 32 24.7-13 12 033.227222.9443G3.227+22.945
IRAS 16296-13050.200ENG15+OH +SiO FRA94
917 09 35.2-26 40 18357.46997.8878G357.470+7.888
IRAS 17064-26360.200ENG15-OH -SiO FRA94
1017 15 29-29 34 00355.85945.1472G355.859+5.147
IRAS 17123-29300.200ENG15-OH FRA94
1118 23 36.9-30 25 532.7190-7.9337G2.719-7.934
IRAS 18204-30270.200ENG15-OH -SiO FRA94
1218 24 2.4-24 57 477.6618-5.5213G7.662-5.521
IRAS 18209-24590.200ENG15-OH +SiO FRA94
1318 25 30.1-24 53 437.8752-5.7845G7.875-5.784
IRAS 18224-24550.200ENG15-OH FRA94
1418 31 18.5-25 34 067.8708-7.2601G7.871-7.260
IRAS 18282-25360.200ENG15-OH +SiO FRA94
1518 37 12.7-23 55 189.9601-7.7256G9.960-7.726
IRAS 18341-23570.200ENG15-OH +SiO FRA94
1617 09 35.2-26 40 18357.46997.8878G357.470+7.888
IRAS 17064-26360.200ENG15-OH -SiO FRA94
1717 15 29-29 34 00355.85945.1472G355.859+5.147
IRAS 17123-29300.200ENG15-OH FRA94
1818 23 36.9-30 25 532.7190-7.9337G2.719-7.934
IRAS 18204-30270.200ENG15-OH -SiO FRA94
1918 24 2.4-24 57 477.6618-5.5213G7.662-5.521
IRAS 18209-24590.200ENG15-OH +SiO FRA94
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  • Distribution of sources in all sky (l,b)

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  • Distribution of sources in all sky using Aladin

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  • 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 FRA94

    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 FRA94 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