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KAL96 - The Observations of Methanol at 36 GHz in Pushchino

Short title: Kalenskii et al. (1996)
Authors: Kalenskii, S. V. Slysh, V. I. Val'tts, I. E. Dzura, A. M.
Journal: Poster Presentations, IAU Symposium 170, CO: Twenty-five Years of Millimeter-wave Spectroscopy, 29 May-2 June, 1996. Tucson, Arizona. Sponsored by IAU and URSI, National Radio Astronomy Observatory, Submillimeter Telescope Observatory., p.49
Bibcode: 1996IAUS..170P..49K

Detection table from Kalenskii et al. (1996)

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ID Obs. RA Obs. Dec l b Group id Source name Line Vpeak FWHM Ta Telescope Beam Detection Class Dist. (parallax)
(J2000) (J2000) (deg.) (deg.) CH3OH (class I) (km/s) (km/s) (K) (arcsec) Yes/No (kpc)
100 52 25+56 33 53.3123.0675-6.3067G123.066-6.309
00494+561736 GHz (I); -31.2(0.2)3.3(0.5)0.33(0.04)RT22_PRAO120+H2O +CH3OH I +CH3OH II SFR
205 46 52.1+00 20 23205.1044-14.1659G205.112-14.173
05443-001936 GHz (I); 15.2(0.48)7.0(1.0)0.1(0.02)RT22_PRAO120-H2O +CH3OH I SFR_MIXED
317 45 39.7-29 00 29.6359.9433-0.0454G359.9444-0.0464
17424-285936 GHz (I); 28.8(4.2)24.2(15.4)0.52(0.06)RT22_PRAO120+H2O +CH3OH I -CH3OH II +OH SFR_MIXED
17 45 39.7-29 00 29.6359.9433-0.0454G359.9444-0.0464
17424-285936 GHz (I); 49.1(1.4)14.4(5.4)0.95(0.21)RT22_PRAO120+H2O +CH3OH I -CH3OH II +OH SFR_MIXED
517 46 26.6-28 56 11.20.0936-0.1541G0.0937-0.1544
17432-285536 GHz (I); 51.9(0.6)10.5(1.6)0.41(0.06)RT22_PRAO120+CH3OH I -CH3OH II SFR
617 46 31.3-28 42 20.80.2995-0.0488G0.2995-0.0488
17433-284136 GHz (I); 34.8(1.7)14.6(4.0)0.29(0.06)RT22_PRAO120+CH3OH I SFR_MIXED
717 50 14.6-28 54 2.60.5533-0.8478G0.546-0.852
17470-285336 GHz (I); 17.3(0.5)7.2(1.4)0.53(0.08)RT22_PRAO120+H2O +CH3OH I +CH3OH II +OH SFR
818 08 35.9-19 52 2.910.46480.0334G10.472+0.027
18056-195236 GHz (I); 70.2(0.9)6.8(2.0)0.18(0.05)RT22_PRAO120+H2O +CH3OH I +CH3OH II +OH SFR
918 17 57.1-12 07 21.718.34021.7722G18.340+1.772
18151-120836 GHz (I); 30.2(0.2)1.5(0.2)0.29(0.04)RT22_PRAO120+H2O +CH3OH I +CH3OH II SFR
1018 18 54.9-16 47 49.714.3324-0.6457G14.332-0.642
14.33-0.6436 GHz (I); 22.0(0.3)3.7(0.8)1.33(0.24)RT22_PRAO120+H2O +CH3OH I +CH3OH II SFR
1118 20 23.1-16 11 49.215.0279-0.6731G15.033-0.674
M17(2)36 GHz (I); 18.2(0.4)3.0(0.8)0.45(0.10)RT22_PRAO120+H2O +CH3OH I +CH3OH II +OH GALAXY
1218 46 11.8-02 39 3.929.9753-0.0438G29.975-0.047
29.98-0.0436 GHz (I); 102.6(0.4)4.0(0.5)0.11(0.01)RT22_PRAO120+H2O +CH3OH I +CH3OH II +OH SFR
1318 47 34.2-01 12 3831.41360.3084G31.412+0.307
18449-011536 GHz (I); 97.8(0.2)3.4(0.5)0.70(0.08)RT22_PRAO120+H2O +CH3OH I +CH3OH II +OH SFR
1418 48 01-01 54 49.130.8389-0.1117G30.843-0.112
1845+015836 GHz (I); 98.9(0.3)4.9(0.7)0.13(0.03)RT22_PRAO120+H2O +CH3OH I +CH3OH II +OH SFR
1518 49 34.5-01 29 8.431.3974-0.2631G31.396-0.257
18469-013236 GHz (I); 84.6(0.2)3.4(0.5)0.42(0.05)RT22_PRAO120+H2O +CH3OH I +CH3OH II +OH SFR
1618 56 10.8+07 53 14.140.49422.5408G40.494+2.541
18537+074936 GHz (I); 31.7(0.2)4.2(1.2)1.06(0.08)RT22_PRAO120+H2O +CH3OH I -CH3OH II SFR
1719 43 11.4+23 43 5459.78080.0630G59.783+0.064
59.78+0.0636 GHz (I); 22.3(0.4)3.6(0.5)0.25(0.05)RT22_PRAO120+H2O +CH3OH I +CH3OH II +OH SFR
1819 46 20.5+24 35 24.460.8837-0.1303G60.884-0.129
19442+242736 GHz (I); 23.0(0.2)2.7(0.4)0.26(0.03)RT22_PRAO120+H2O +CH3OH I -CH3OH II SFR
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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 KAL96

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

  • Distribution of sources from KAL96 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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