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MAC92B - Search and detection of 5 1-6 0A+ -methanol masers towards southern galactic star-forming regions.

Short title: MacLeod et al. (1992b)
Authors: MacLeod, G. C.Gaylard, M. J.Nicolson, G. D.
Journal: Monthly Notices of the Royal Astronomical Society, Vol. 254, 1P-6P (1992)
Bibcode: 1992MNRAS.254P...1M

Detection table from MacLeod et al. (1992b)

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ID Obs. RA Obs. Dec l b Group id Source name Image Line Vrange Fpeak ∫F dv Telescope RMS Beam Detection Class Dist. (parallax) Date
(J2000) (J2000) (deg.) (deg.) CH3OH (class II) (km/s) (Jy) (Jy*km/s) (Jy) (arcsec) Yes/No (kpc)
111 11 57.9-61 19 5.6291.2869-0.7159G291.274-0.709
291.29-0.723 Image 6.6 GHz (II); -31;-2973 (6)90 (5)HartRAO4.000420+H2O -CH3OH I +CH3OH II SFR1991 Sep 27 - Oct 5
213 11 20.2-62 45 25.5305.20690.0267G305.200+0.019
305.21+0.033 Image 6.6 GHz (II); -34;-3250 (4)38 (2)HartRAO4.000420+H2O -CH3OH I +CH3OH II +OH SFR1991 Sep 27 - Oct 5
313 11 12-62 34 46.7305.20480.2049G305.208+0.206
305.20+0.213 Image 6.6 GHz (II); -39;-36400 (24)289 (15)HartRAO4.000420+H2O +CH3OH I +CH3OH II +OH SFR1991 Sep 27 - Oct 5
413 43 4.6-62 08 50.1308.92340.1223G308.918+0.123
308.92+0.122 Image 6.6 GHz (II); -56;-5244 (4)36 (3)HartRAO4.000420+H2O -CH3OH I +CH3OH II +OH SFR1991 Sep 27 - Oct 5
513 50 42.7-61 35 39.4309.92050.4706G309.921+0.479
309.92+0.483 Image 6.6 GHz (II); -63;-58732 (36)933 (44)HartRAO4.000420-H2O +CH3OH II +OH SFR1991 Sep 27 - Oct 5
614 44 18.5-59 54 59.2316.6420-0.0837G316.640-0.087
316.64-0.083 Image 6.6 GHz (II); -23;-19108 (9)77 (4)HartRAO4.000420+H2O +CH3OH II +OH SFR1991 Sep 27 - Oct 5
715 00 58-58 58 39.9318.9545-0.1957G318.948-0.196
318.95-0.203 Image 6.6 GHz (II); -38;-33662 (33)453 (20)HartRAO4.000420+H2O +CH3OH I +CH3OH II +OH SFR1991 Sep 27 - Oct 5
815 29 19.6-56 31 23.4323.4592-0.0793G323.459-0.079
323.46-0.081 Image 6.6 GHz (II); -67;-6716 (3)8 (2)HartRAO4.000420-H2O +CH3OH II +OH SFR1991 Sep 27 - Oct 5
915 31 43.4-56 30 26.1323.7400-0.2544G323.740-0.263
323.77-0.213 Image 6.6 GHz (II); -54;-472721 (125)3875 (175)HartRAO4.000420+H2O +CH3OH I +CH3OH II +OH SFR_MIXED1991 Sep 27 - Oct 5
1015 49 21-53 45 31.1327.40210.4384G327.402+0.444
327.40+0.453 Image 6.6 GHz (II); -84;-8170 (5)95 (5)HartRAO4.000420+H2O -CH3OH I +CH3OH II +OH SFR1991 Sep 27 - Oct 5
1115 57 57.3-53 58 45.3328.2413-0.5377G328.237-0.547
328.24-0.542 Image 6.6 GHz (II); -50;-46442 (20)750 (35)HartRAO4.000420+H2O +CH3OH I +CH3OH II +OH SFR1991 Sep 27 - Oct 5
1215 55 47.4-52 43 8.3328.80600.6344G328.809+0.633
328.81+0.643 Image 6.6 GHz (II); -47;-43363 (18)385 (18)HartRAO4.000420+H2O +CH3OH I +CH3OH II +OH SFR1991 Sep 27 - Oct 5
1316 00 34.5-53 12 37.4329.0368-0.2067G329.031-0.200
329.04-0.213 Image 6.6 GHz (II); -40;-35161 (20)196 (12)HartRAO4.000420+H2O +CH3OH I +CH3OH II +OH SFR1991 Sep 27 - Oct 5
1416 11 29.1-51 42 16.6331.2792-0.1966G331.278-0.188
331.28-0.203 Image 6.6 GHz (II); -86;-77184 (16)264 (14)HartRAO4.000420+H2O +CH3OH I +CH3OH II +OH SFR1991 Sep 27 - Oct 5
1516 29 49-48 16 8.9335.78880.1674G335.789+0.174
335.79+0.173 Image 6.6 GHz (II); -51;-46100 (15)268 (14)HartRAO4.000420+H2O +CH3OH I +CH3OH II +OH SFR1991 Sep 27 - Oct 5
1616 38 10.4-47 05 16.9337.6107-0.0647G337.613-0.060
337.61-0.072 Image 6.6 GHz (II); -44;-4124 (4)31 (3)HartRAO4.000420+H2O +CH3OH II +OH SFR1991 Sep 27 - Oct 5
1716 38 29.6-47 00 51.6337.7019-0.0560G337.705-0.053
337.71-0.062 Image 6.6 GHz (II); -55;-49153 (9)248 (12)HartRAO4.000420+H2O +CH3OH I +CH3OH II +OH SFR1991 Sep 27 - Oct 5
1816 52 4.6-46 08 30.5339.8847-1.2580G339.884-1.259
339.88-1.263 Image 6.6 GHz (II); -40;-311460 (70)2658 (120)HartRAO4.000420+H2O +CH3OH I +CH3OH II +OH SFR1991 Sep 27 - Oct 5
1916 50 14.6-44 42 31340.7836-0.0963G340.785-0.096
340.78-0.103 Image 6.6 GHz (II); -107;-104590 (30)376 (18)HartRAO4.000420+H2O +CH3OH I +CH3OH II +OH SFR1991 Sep 27 - Oct 5
2016 52 17.8-44 26 52.4341.2176-0.2119G341.218-0.212
341.21-0.212 Image 6.6 GHz (II); -50;-37134 (10)228 (12)HartRAO4.000420+H2O +CH3OH I +CH3OH II +OH SFR1991 Sep 27 - Oct 5
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  • Distribution of sources in all sky (l,b)

    0

  • 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 MAC92B

    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 MAC92B 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

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    2MASS K

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