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GAY94 - 12.2-GHz methanol and 1.6-GHz hydroxyl masers associated with new 6.7-GHz methanol masers.

Short title: Gaylard et al. (1994)
Authors: Gaylard, M. J.MacLeod, G. C.van der Walt, D. J.
Journal: Monthly Notices of the Royal Astronomical Society, Vol. 269, 257-264 (1994)
Bibcode: 1994MNRAS.269..257G

Detection table from Gaylard et al. (1994)

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ID Obs. RA Obs. Dec l b Group id Source name Image Descr. Line Vrange Vpeak FWHM Fpeak Telescope RMS Beam Detection Class Dist. (parallax) Date
(J2000) (J2000) (deg.) (deg.) CH3OH (class II) (km/s) (km/s) (km/s) (Jy) (Jy) (arcsec) Yes/No (kpc)
110 48 4.5-58 26 59.2287.37110.6447G287.371+0.644
10460-5811 Image 12 GHz (II); -228 (2)HartRAO3.300240+H2O -CH3OH I +CH3OH II +OH SFR1992 Oct-1993 Aug
213 51 57.8-61 15 45.9310.14230.7588G310.144+0.760
13484-6100 Image 12 GHz (II); -58;-55-58-55114 (5)HartRAO3.300240+H2O +CH3OH I +CH3OH II +OH SFR1992 Oct-1993 Aug
314 43 15.5-60 17 17.2316.3675-0.3664G316.361-0.363
14394-6004 Image 12 GHz (II); 3.68 (2)HartRAO3.300240+H2O +CH3OH II +OH SFR1992 Oct-1993 Aug
415 16 10.9-58 12 15.6321.0571-0.5203G321.033-0.485
15122-5801 Image Descr 12 GHz (II); -67;-65-67-6532 (3)HartRAO3.300240+H2O +CH3OH II +OH SFR1992 Oct-1993 Aug
516 02 14.6-52 38 33329.59910.0570G329.599+0.057
15584-5230 Image 12 GHz (II); -61;-59-61-5911 (2)HartRAO3.300240+CH3OH II SFR1992 Oct-1993 Aug
616 05 40.9-49 11 29.7332.29322.2814G332.294+2.280
16019-4903 Image 12 GHz (II); -25;-22-25-2260 (3)HartRAO3.300240+H2O +CH3OH II +OH SFR1992 Oct-1993 Aug
716 12 16-51 35 13.5331.4481-0.1936G331.442-0.187
16084-5127 Image 12 GHz (II); -8854 (1.5)HartRAO3.300240+H2O +CH3OH I +CH3OH II +OH SFR1992 Oct-1993 Aug
816 35 7.9-48 46 16.5336.0218-0.8187G336.018-0.826
16313-4840 Image Descr 12 GHz (II); -39.6254 (03)HartRAO3.300240+H2O +CH3OH I +CH3OH II +OH SFR1992 Oct-1993 Aug
917 23 29.2-37 01 38.4350.6895-0.4909G350.686-0.491
17200-3658 Image 12 GHz (II); -148.54 (1.5)HartRAO3.300240+H2O +CH3OH I +CH3OH II +OH SFR1992 Oct-1993 Aug
1017 46 9.8-28 23 29.40.52710.1817G0.5271+0.1818
17430-2822 Image 12 GHz (II); -3;2-3254 (1.5)HartRAO3.300240+H2O +CH3OH II SFR1992 Oct-1993 Aug
1117 47 8.6-28 46 18.10.3138-0.1995G0.3138-0.1992
17439-2845 Image 12 GHz (II); 14;16141634 (01)HartRAO3.300240+CH3OH II +OH SFR1992 Oct-1993 Aug
1218 01 57.1-23 12 37.16.7935-0.2556G6.794-0.256
17589-2312 Image Descr 12 GHz (II); 15;16151631 (3)HartRAO3.300240+H2O +CH3OH I +CH3OH II +OH SFR1992 Oct-1993 Aug
1318 16 22.3-19 41 19.911.4994-1.4848G11.499-1.485
18134-1942 Image 12 GHz (II); 6;1661692 (5)HartRAO3.300240+H2O -CH3OH I +CH3OH II SFR1992 Oct-1993 Aug
1418 35 10.7-08 17 55.623.6995-0.1942G23.706-0.198
18324-0820 Image 12 GHz (II); 78;80788014 (2)HartRAO3.300240+H2O -CH3OH I +CH3OH II +OH SFR1992 Oct-1993 Aug
1518 38 51.7-06 25 0.625.7905-0.1407G25.791-0.141
18361-0627 Image 12 GHz (II); 90;92909213 (2)HartRAO3.300240+H2O +CH3OH II UNK1992 Oct-1993 Aug
1618 44 18.5-04 17 53.128.2949-0.3766G28.295-0.377
18416-0420 Image 12 GHz (II); 81;82818213 (2)HartRAO3.300240+H2O +CH3OH I +CH3OH II +OH SFR1992 Oct-1993 Aug
1718 49 36.5-00 45 50.232.04340.0587G32.045+0.059
18470-0049 Image 12 GHz (II); 98;1019810118 (2)HartRAO3.300240+H2O +CH3OH I +CH3OH II +OH SFR1992 Oct-1993 Aug
1818 54 13.8+04 41 31.737.42661.5183G37.427+1.518
18517+0437 Image 12 GHz (II); 41154 (02)HartRAO3.300240+H2O +CH3OH I +CH3OH II SFR1992 Oct-1993 Aug
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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

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    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 GAY94

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    Longitude-Velocity Map is taken form Dame, Hartmann & Thaddeus (2001)

  • Distribution of sources from GAY94 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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