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Data: CH3OH_I

KAL06 - The detection of class I methanol masers towards regions of low-mass star formation

Short title: Kalenskii et al. (2006)
Authors: Kalenskii, S. V. Promyslov, V. G. Slysh, V. I. Bergman, P. Winnberg, A.
Journal: Astronomy Reports, vol. 50, Issue 4, p.289-297
Bibcode: 2006ARep...50..289K

PDF: KAL06.pdf

Detection table from Kalenskii et al. (2006)

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ID Obs. RA Obs. Dec l b Source name Image Line Thermal Vpeak FWHM Ta ∫Ta dv Telescope Beam Date
(J2000) (J2000) (deg.) (deg.) CH3OH (class I) line mark (km/s) (km/s) (K) (K*km/s) (arcsec)
103 29 10.3+31 13 31.2158.3947-20.5748NGC 1333-IRS4A2(-1)->1(-1)_E
*6.22(0.29)5.31(0.37)0.25(0.05)ONSALA39December 6-9, 2004
203 29 10.3+31 13 31.2158.3947-20.5748NGC 1333-IRS4A2(-1)->1(-1)_E
*7.69(0.03)1.14(0.04)0.79(0.07)ONSALA39December 6-9, 2004
303 29 10.3+31 13 31.2158.3947-20.5748NGC 1333-IRS4A84 GHz (I)
3.78(0.16)7.19(0.31)0.211.60(0.12)ONSALA44December 6-9, 2004
403 29 10.3+31 13 31.2158.3947-20.5748NGC 1333-IRS4A Image 84 GHz (I)
6.95(0.04)0.67(0.13)0.230.16(0.04)ONSALA44December 6-9, 2004
503 29 10.3+31 13 31.2158.3947-20.5748NGC 1333-IRS4A84 GHz (I)
6.42(0.10)2.31(0.17)0.260.64(0.03)ONSALA44December 6-9, 2004
603 29 10.3+31 13 31.2158.3947-20.5748NGC 1333-IRS4A44 GHz (I)
6.65(0.13)1.59(0.22)0.0950.16(0.02)ONSALA82December 6-9, 2004
703 29 10.3+31 13 31.2158.3947-20.5748NGC 1333-IRS4A44 GHz (I)
7.51(0.02)0.33(0.05)0.250.09(0.02)ONSALA82December 6-9, 2004
803 29 10.3+31 13 31.2158.3947-20.5748NGC 1333-IRS4A95 GHz (I)
4.38(0.78)8.93(1.49)0.111.01(0.11)ONSALA39December 6-9, 2004
903 29 10.3+31 13 31.2158.3947-20.5748NGC 1333-IRS4A95 GHz (I)
7.32(0.03)0.94(0.14)0.450.44(0.06)ONSALA39December 6-9, 2004
1003 29 12+31 13 9.1158.4038-20.5760NGC 1333-IRS4B2(-1)->1(-1)_E
*7.74(0.07)1.24(0.07)0.58(0.07)ONSALA39December 6-9, 2004
1103 29 12+31 13 9.1158.4038-20.5760NGC 1333-IRS4B84 GHz (I)
4.72(0.15)8.77(0.29)0.292.70(0.09)ONSALA44December 6-9, 2004
1203 29 12+31 13 9.1158.4038-20.5760NGC 1333-IRS4B84 GHz (I)
6.86(0.04)1.59(0.10)0.430.73(0.05)ONSALA44December 6-9, 2004
1303 29 12+31 13 9.1158.4038-20.5760NGC 1333-IRS4B44 GHz (I)
7.10(0.07)1.83(0.21)0.160.32(0.03)ONSALA82December 6-9, 2004
1403 29 12+31 13 9.1158.4038-20.5760NGC 1333-IRS4B95 GHz (I)
5.36(0.30)9.31(0.57)0.121.15(0.07)ONSALA39December 6-9, 2004
1503 29 12+31 13 9.1158.4038-20.5760NGC 1333-IRS4B95 GHz (I)
6.08(0.07)0.76(0.20)0.20.16(0.04)ONSALA39December 6-9, 2004
1603 29 12+31 13 9.1158.4038-20.5760NGC 1333-IRS4B95 GHz (I)
7.16(0.04)0.76(0.08)0.40.33(0.03)ONSALA39December 6-9, 2004
1703 29 00+31 14 18.8158.3549-20.5864NGC 1333-IRS2 Image 2(-1)->1(-1)_E
*9.51(0.14)5.56(0.16)0.45(0.03)ONSALA39December 6-9, 2004
1803 29 00+31 14 18.8158.3549-20.5864NGC 1333-IRS22(-1)->1(-1)_E
*7.53(0.05)1.42(0.06)0.30(0.03)ONSALA39December 6-9, 2004
1903 29 00+31 14 18.8158.3549-20.5864NGC 1333-IRS284 GHz (I)
10.14(0.04)5.46(0.10)0.925.32(0.09)ONSALA44December 6-9, 2004
2003 29 00+31 14 18.8158.3549-20.5864NGC 1333-IRS244 GHz (I)
10.83(0.17)7.88(0.45)0.161.33(0.06)ONSALA82December 6-9, 2004
2103 29 00+31 14 18.8158.3549-20.5864NGC 1333-IRS2 Image 95 GHz (I)
9.97(0.28)8.38(0.85)0.110.98(0.08)ONSALA39December 6-9, 2004
2205 46 7.5-00 14 13.7205.5393-14.6018HH 25MMS2(-1)->1(-1)_E
*10.25(0.05)3.56(0.07)0.51(0.02)ONSALA39December 6-9, 2004
2305 46 7.5-00 14 13.7205.5393-14.6018HH 25MMS84 GHz (I)
10.53(0.07)2.87(0.17)0.531.63(0.08)ONSALA44December 6-9, 2004
2405 46 7.5-00 14 13.7205.5393-14.6018HH 25MMS44 GHz (I)
10.42(0.01)0.48(0.04)0.520.27(0.02)ONSALA82December 6-9, 2004
2505 46 7.5-00 14 13.7205.5393-14.6018HH 25MMS95 GHz (I)
9.97(0.36)5.60(0.80)0.140.81(0.11)ONSALA39December 6-9, 2004
2605 46 7.5-00 14 13.7205.5393-14.6018HH 25MMS95 GHz (I)
10.14(0.03)0.53(0.06)0.540.31(0.04)ONSALA39December 6-9, 2004
2720 39 8.1+68 01 13.4102.641215.7839L1157-B12(-1)->1(-1)_E
*0.43(0.05)5.00(0.05)0.75(0.02)ONSALA39December 6-9, 2004
2820 39 8.1+68 01 13.4102.641215.7839L1157-B184 GHz (I)
0.10(0.04)4.81(0.09)0.94.61(0.07)ONSALA44December 6-9, 2004
2920 39 8.1+68 01 13.4102.641215.7839L1157-B144 GHz (I)
0.69(0.08)3.82(0.24)0.170.60(0.03)ONSALA82December 6-9, 2004
3020 39 8.1+68 01 13.4102.641215.7839L1157-B144 GHz (I)
0.75(0.01)0.37(0.03)0.310.12(0.01)ONSALA82December 6-9, 2004
3120 39 8.1+68 01 13.4102.641215.7839L1157-B195 GHz (I)
-0.18(0.15)5.19(0.33)0.291.61(0.09)ONSALA39December 6-9, 2004
3220 39 9.3+68 00 43.5102.635315.7776L1157-B22(-1)->1(-1)_E
*1.30(0.06)4.00(0.07)0.55(0.02)ONSALA39December 6-9, 2004
3320 39 9.3+68 00 43.5102.635315.7776L1157-B244 GHz (I)
0.04(0.38)5.29(0.43)0.110.61(0.09)ONSALA82December 6-9, 2004
3420 39 9.3+68 00 43.5102.635315.7776L1157-B244 GHz (I)
1.53(0.14)2.17(0.49)0.120.28(0.11)ONSALA82December 6-9, 2004
3520 39 9.3+68 00 43.5102.635315.7776L1157-B244 GHz (I)
0.72(0.03)0.36(0.08)0.110.04(0.01)ONSALA82December 6-9, 2004
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  • Distribution of sources in all sky (l,b)

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  • 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 KAL06

    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 KAL06 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