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FON10 - Class I and Class II methanol masers in high-mass star-forming regions

Short title: Fontani et al. (2010)
Authors: Fontani, F. Cesaroni, R. Furuya, R. S.
Journal: Astronomy and Astrophysics, Volume 517, id.A56, 24 pp.
Bibcode: 2010A&A...517A..56F

Detection table from Fontani et al. (2010)

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ID Obs. RA Obs. Dec l b Group id Source name Line Vpeak FWHM Fpeak ∫F dv Telescope Beam Detection Class Dist. (parallax) Date
(J2000) (J2000) (deg.) (deg.) CH3OH (class I) (km/s) (km/s) (Jy) (Jy*km/s) (arcsec) Yes/No (kpc)
105 20 16.1+36 37 21170.6566-0.2692G170.657-0.269
05168+363444 GHz (I); -4.9 (0.2)1.3 (0.4)0.81.12 (0.2)NRO38+H2O +CH3OH I -CH3OH II SFRApril 2002
205 51 10.6+25 46 14183.3482-0.5770G183.348-0.577
05480+254544 GHz (I); -9.79 (0.02)0.77 (0.05)4.083.3 (0.1)NRO38+H2O +CH3OH I +CH3OH II SFR_MIXEDApril 2002
306 04 34.2+30 30 39180.71274.3468G180.713+4.347
06013+303044 GHz (I); 16.4 (0.7)5 (1.5)0.512.7 (0.6)NRO38-H2O +CH3OH I -CH3OH II EVOLVEDApril 2002
418 11 51.3-17 31 2912.88870.4897G12.889+0.490
18089-173244 GHz (I); 31.94 (0.01)0.86 (0.04)11.810.9 (0.4)NRO38+H2O +CH3OH I +CH3OH II +OH SFRApril 2002
518 17 57.1-12 07 2218.34011.7722G18.340+1.772
18151-120844 GHz (I); 30.5 (0.1)1.5 (0.3)1.342.2 (0.2)NRO38+H2O +CH3OH I +CH3OH II SFRApril 2002
18 17 57.1-12 07 2218.34011.7722G18.340+1.772
18151-120844 GHz (I); 33.8 (0.2)2.1 (0.5)0.892.0 (0.4)NRO38+H2O +CH3OH I +CH3OH II SFRApril 2002
718 18 53-16 47 3914.3314-0.6376G14.332-0.642
18159-164844 GHz (I); 13.2 (0.1)0.9 (0.1)3.954.0 (0.6)NRO38+H2O +CH3OH I +CH3OH II SFRApril 2002
18 18 53-16 47 3914.3314-0.6376G14.332-0.642
18159-164844 GHz (I); 19.5 (0.1)1.0 (0.1)10.0110.9 (0.6)NRO38+H2O +CH3OH I +CH3OH II SFRApril 2002
18 18 53-16 47 3914.3314-0.6376G14.332-0.642
18159-164844 GHz (I); 20.9 (0.1)1.0 (0.1)6.9715.8 (0.6)NRO38+H2O +CH3OH I +CH3OH II SFRApril 2002
18 18 53-16 47 3914.3314-0.6376G14.332-0.642
18159-164844 GHz (I); 22.9 (0.1)0.9 (0.1)32.1131.4 (0.6)NRO38+H2O +CH3OH I +CH3OH II SFRApril 2002
18 18 53-16 47 3914.3314-0.6376G14.332-0.642
18159-164844 GHz (I); 23.9 (0.1)0.6 (0.1)27.918.5 (0.6)NRO38+H2O +CH3OH I +CH3OH II SFRApril 2002
1218 34 19.8-05 59 4425.64711.0533G25.649+1.050
18316-060244 GHz (I); 42.060 (0.008)0.62 (0.02)9.886.6 (0.1)NRO38+H2O +CH3OH I +CH3OH II +OH SFRApril 2002
18 34 19.8-05 59 4425.64711.0533G25.649+1.050
18316-060244 GHz (I); 43.10 (0.04)0.70 (0.09)2.071.6 (0.2)NRO38+H2O +CH3OH I +CH3OH II +OH SFRApril 2002
18 34 19.8-05 59 4425.64711.0533G25.649+1.050
18316-060244 GHz (I); 44.52 (0.09)1.6 (0.3)1.672.9 (0.4)NRO38+H2O +CH3OH I +CH3OH II +OH SFRApril 2002
1518 38 40.3-05 35 0626.50800.2829G26.510+0.282
18360-053744 GHz (I); 102.4 (0.1)2.83 (0.2)2.236.7 (0.4)NRO38+H2O +CH3OH I -CH3OH II +OH SFRApril 2002
18 38 40.3-05 35 0626.50800.2829G26.510+0.282
18360-053744 GHz (I); 106.4 (0.3)1.9 (0.7)0.741.6 (0.4)NRO38+H2O +CH3OH I -CH3OH II +OH SFRApril 2002
1718 53 17.4+01 24 5534.40260.2333G34.403+0.232
18507+012144 GHz (I); 60.33 (0.04)1.3 (0.1)710.0 (0.4)NRO38+H2O +CH3OH I +CH3OH II +OH SFR_MIXEDApril 2002
1818 54 13.8+04 41 3237.42671.5182G37.427+1.518
18517+043744 GHz (I); 43.97 (0.05)1.1 (0.1)2.73.1 (0.2)NRO38+H2O +CH3OH I +CH3OH II SFRApril 2002
1919 06 47.6+07 31 3841.37640.0379G41.377+0.038
19043+072644 GHz (I); 58.69 (0.03)0.65 (0.09)3.522.5 (0.2)NRO38+H2O +CH3OH I -CH3OH II SFRApril 2002
19 06 47.6+07 31 3841.37640.0379G41.377+0.038
19043+072644 GHz (I); 59.89 (0.08)0.7 (0.2)1.311.1 (0.2)NRO38+H2O +CH3OH I -CH3OH II SFRApril 2002
2119 11 15.9+09 07 2743.3035-0.2073G43.305-0.209
19088+090244 GHz (I); 58.67 (0.07)2.2 (0.2)210 (1)NRO38+H2O +CH3OH I -CH3OH II SFRApril 2002
2219 40 59.3+24 04 3959.83160.6713G59.833+0.671
19388+235744 GHz (I); 35.4 (0.2)1.6 (0.4)1.071.8 (0.4)NRO38+H2O +CH3OH I +CH3OH II +OH SFRApril 2002
2320 07 6.7+27 28 5365.7802-2.6122G65.780-2.612
20050+272044 GHz (I); 6.6 (0.1)1.8 (0.3)1.092.0 (0.2)NRO38+H2O +CH3OH I -CH3OH II SFR_MIXEDApril 2002
2420 08 9.7+35 59 2073.06151.7967G73.062+1.796
20062+355044 GHz (I); 0.60 (0.06)1.0 (0.1)2.362.5 (0.2)NRO38+H2O +CH3OH I +CH3OH II +OH SFR_MIXEDApril 2002
2520 14 26+41 13 3278.12213.6328G78.122+3.633
20126+410444 GHz (I); -2.43 (0.04)2.0 (0.1)4.178.9 (0.4)NRO38+H2O +CH3OH I +CH3OH II +OH SFRApril 2002
2620 20 39.3+39 37 5277.46221.7595G77.462+1.760
20188+392844 GHz (I); 3 (1)3 (2)0.762 (1)NRO38+H2O +CH3OH I -CH3OH II SFRApril 2002
2721 40 42.3+58 16 1099.98244.1698G99.982+4.170
21391+580244 GHz (I); -0.49 (0.02)0.73 (0.08)5.334.2 (0.2)NRO38+H2O +CH3OH I +CH3OH II GALAXYApril 2002
21 40 42.3+58 16 1099.98244.1698G99.982+4.170
21391+580244 GHz (I); 6.6 (0.1)2.3 (0.3)2.255.4 (0.4)NRO38+H2O +CH3OH I +CH3OH II GALAXYApril 2002
2922 52 38.6+60 00 56108.59570.4925G108.595+0.492
22506+594444 GHz (I); -51.3 (0.1)1.6 (0.6)1.813 (1)NRO38+H2O +CH3OH I +CH3OH II SFR_MIXEDApril 2002
22 52 38.6+60 00 56108.59570.4925G108.595+0.492
22506+594444 GHz (I); -48 (1)5 (2)0.84 (2)NRO38+H2O +CH3OH I +CH3OH II SFR_MIXEDApril 2002
3100 44 57.6+55 47 18122.0145-7.0719G122.014-7.072
00420+553044 GHz (I); -48.8 (0.3)2.0 (0.5)0.81.6 (0.4)NRO38+H2O +CH3OH I -CH3OH II SFRApril 2002
3218 04 53.9-24 26 416.0501-1.4494G6.050-1.449
18018-242644 GHz (I); 11.280 (0.003)0.669 (0.002)339241.1 (0.4)NRO38+H2O +CH3OH I +CH3OH II +OH SFRApril 2002
3318 05 25.4-21 19 418.8273-0.0292G8.832-0.028
18024-211944 GHz (I); 0.31 (0.02)1.28 (0.05)7.3410.0 (0.4)NRO38+H2O +CH3OH I +CH3OH II +OH SFRApril 2002
18 05 25.4-21 19 418.8273-0.0292G8.832-0.028
18024-211944 GHz (I); 2.7 (0.1)2.3 (0.3)1.43.1 (0.4)NRO38+H2O +CH3OH I +CH3OH II +OH SFRApril 2002
3518 17 24.4-17 22 1313.6568-0.5998G13.657-0.600
18144-172344 GHz (I); 48.590 (0.005)1.54 (0.01)25.642.1 (0.2)NRO38+H2O +CH3OH I +CH3OH II +OH SFRApril 2002
3618 19 7.5-16 11 2114.8919-0.4026G14.891-0.404
18162-161244 GHz (I); 62.80 (0.03)0.84 (0.07)3.25.1 (0.2)NRO38+H2O +CH3OH I -CH3OH II SFR_MIXEDApril 2002
3718 42 18.8-04 28 3727.9084-0.0159G27.908-0.016
18396-043144 GHz (I); 97.6 (0.1)1.0 (0.3)11.0 (0.2)NRO38+H2O +CH3OH I -CH3OH II SFRApril 2002
3819 11 37.4+08 46 3043.0348-0.4473G43.038-0.453
19092+084144 GHz (I); 59.07 (0.4)5.7 (0.7)0.654.0 (0.4)NRO38+H2O +CH3OH I +CH3OH II +OH SFRApril 2002
3923 40 53.2+61 10 21114.5307-0.5432G114.531-0.543
23385+605344 GHz (I); -50.6 (0.3)3.2 (0.7)0.92.9 (0.4)NRO38+H2O +CH3OH I -CH3OH II SFRApril 2002
4005 51 10.6+25 46 14183.3482-0.5770G183.348-0.577
05480+254595 GHz (I); -10.6 (0.1)1.3 (0.3)2.23.1 (0.6)NRO18+H2O +CH3OH I +CH3OH II SFR_MIXEDApril 2002
4118 11 51.3-17 31 2912.88870.4897G12.889+0.490
18089-173295 GHz (I); 31.38 (0.02)0.45 (0.05)5.52.7 (0.4)NRO18+H2O +CH3OH I +CH3OH II +OH SFRApril 2002
18 11 51.3-17 31 2912.88870.4897G12.889+0.490
18089-173295 GHz (I); 32.4 (0.2)3.2 (0.4)4.214 (2)NRO18+H2O +CH3OH I +CH3OH II +OH SFRApril 2002
4318 18 53-16 47 3914.3314-0.6376G14.332-0.642
18159-164895 GHz (I); 20.1 (0.1)1.6 (0.4)2.74.7 (0.8)NRO18+H2O +CH3OH I +CH3OH II SFRApril 2002
18 18 53-16 47 3914.3314-0.6376G14.332-0.642
18159-164895 GHz (I); 22.56 (0.06)1.4 (0.1)5.27.6 (0.6)NRO18+H2O +CH3OH I +CH3OH II SFRApril 2002
4518 34 19.8-05 59 4425.64711.0533G25.649+1.050
18316-060295 GHz (I); 41.63 (0.05)0.5 (0.1)2.11.1 (0.2)NRO18+H2O +CH3OH I +CH3OH II +OH SFRApril 2002
4618 38 40.3-05 35 0626.50800.2829G26.510+0.282
18360-053795 GHz (I); 102.5 (0.1)4.1 (0.4)413.2 (0.8)NRO18+H2O +CH3OH I -CH3OH II +OH SFRApril 2002
4720 14 26+41 13 3278.12213.6328G78.122+3.633
20126+410495 GHz (I); -2.75 (0.08)2.3 (0.2)2.56.0 (0.4)NRO18+H2O +CH3OH I +CH3OH II +OH SFRApril 2002
4821 40 42.3+58 16 1099.98244.1698G99.982+4.170
21391+580295 GHz (I); 12.1 (0.1)1.2 (0.5)22.5 (0.6)NRO18+H2O +CH3OH I +CH3OH II GALAXYApril 2002
4922 52 38.6+60 00 56108.59570.4925G108.595+0.492
22506+594495 GHz (I); -47.1 (0.2)2.4 (0.6)25 (1)NRO18+H2O +CH3OH I +CH3OH II SFR_MIXEDApril 2002
5018 04 53.9-24 26 416.0501-1.4494G6.050-1.449
18018-242695 GHz (I); 10.800 (0.004)0.622 (0.009)5033.5 (0.4)NRO18+H2O +CH3OH I +CH3OH II +OH SFRApril 2002
5118 17 24.4-17 22 1313.6568-0.5998G13.657-0.600
18144-172395 GHz (I); 47.91 (0.03)2.07 (0.08)1226.4 (0.6)NRO18+H2O +CH3OH I +CH3OH II +OH SFRApril 2002
5218 42 18.8-04 28 3727.9084-0.0159G27.908-0.016
18396-043195 GHz (I); 50.37 (0.08)1.24 (0.2)2.93.8 (0.4)NRO18+H2O +CH3OH I -CH3OH II SFRApril 2002
18 42 18.8-04 28 3727.9084-0.0159G27.908-0.016
18396-043195 GHz (I); 57.4 (0.6)7 (1)1.914 (2)NRO18+H2O +CH3OH I -CH3OH II SFRApril 2002
18 42 18.8-04 28 3727.9084-0.0159G27.908-0.016
18396-043195 GHz (I); 61.5 (0.1)1.3 (0.4)2.54 (1)NRO18+H2O +CH3OH I -CH3OH II SFRApril 2002
18 42 18.8-04 28 3727.9084-0.0159G27.908-0.016
18396-043195 GHz (I); 71.3 (0.2)3.4 (0.6)2.28.0 (0.8)NRO18+H2O +CH3OH I -CH3OH II SFRApril 2002
18 42 18.8-04 28 3727.9084-0.0159G27.908-0.016
18396-043195 GHz (I); 130.50 (0.08)0.7 (0.1)2.11.6 (0.2)NRO18+H2O +CH3OH I -CH3OH II SFRApril 2002
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  • Distribution of sources in all sky (l,b)

    0

  • 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 FON10

    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 FON10 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

    Download UKIDSS K FITS
    2MASS K

    Download 2MASS K FITS