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LIE97 - Thermal methanol emission in the DR21 complex. Interferometric maps: a comparison with maser emission.

  Interferometry data

Short title: Liechti & Walmsley (1997)
Authors: Liechti, S. Walmsley, C. M.
Journal: Astronomy and Astrophysics, v.321, p.625-633
Bibcode: 1997A&A...321..625L

Detection table from Liechti & Walmsley (1997)

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ID Obs. RA Obs. Dec RA offset Dec offset l b Group id # Maser spot Source name Image Line Thermal Vpeak Ta Major Minor PA Telescope Beam Detection Class Dist. (parallax) Date
(J2000) (J2000) (mas) (mas) (deg.) (deg.) CH3OH (class I) line mark (km/s) (K) (arcsec) (arcsec) (deg.) (arcsec) Yes/No (kpc)
1+20 39 0.137182+42 22 46.409181.7195370.572829G81.711+0.563
DR 21(OH) Image 2(0)->1(0)_A+; *-5.1 .. -0.28 .. 74IRAM_inter3.5+H2O +CH3OH I +CH3OH II +OH -SiO SFRJune and September 1993
+20 39 0.177568+42 22 45.8114604.325 mas-597.437 mas81.7194800.57263011 (DR 21(OH)-2)DR 21(OH)-1.114 (5)8.1006.500110.000
+20 39 0.35789+42 22 46.22153309.15 mas-187.312 mas81.7199080.57225922 (MM2)DR 21(OH)-0.218 (5)9.6007.80045.000
+20 39 1.18894+42 22 49.068215774.9 mas2659.36 mas81.7220920.57070933 (MM1)DR 21(OH)-3.474 (52)5.4004.30058.000
+20 39 1.69317+42 22 42.896423338.4 mas-3512.41 mas81.7216750.56843444 (DR 21(OH)-4)DR 21(OH)-5.111 (1)7.3004.40046.000
+20 39 0.460639+42 22 40.82724850.38 mas-5581.61 mas81.7189110.57109655DR 21(OH)-0.813 (1)9.3005.30084.000
+20 39 2.07212+42 22 25.617429022.5 mas-20791.4 mas81.7185750.56458966DR 21(OH)-2.48 (2)5.1003.200135.000
+20 38 59.0048+42 22 22.7453-16987.6 mas-23663.5 mas81.7121980.57159977 (DR 21(OH)W-A)DR 21(OH)-1.911 (4)10.6005.00045.000
+20 39 1.85839+42 22 54.405825816.7 mas7997 mas81.7245220.56997588DR 21(OH)-3.99 (3)6.3004.40053.000
+20 38 58.9065+42 22 40.34-18462 mas-6068.85 mas81.7158940.57481199DR 21(OH)-4.511 (2)7.3005.60078.000
+20 39 1.4708+42 22 24.783720002.8 mas-21625.1 mas81.7172650.5659171010DR 21(OH)-3.79 (5)3.7003.40046.000
2+20 38 54.8052+42 19 22.107381.6644970.551354G81.711+0.563
DR 21-W2(0)->1(0)_A+; *-5.3 .. -1.16 .. 12IRAM_inter3.5+H2O +CH3OH I +CH3OH II +OH -SiO SFRJune and September 1993
+20 38 54.8747+42 19 23.71121042.28 mas1602.44 mas81.6649810.55145511DR 21-W-1.99 (2)7.1005.10045.000
+20 38 54.8655+42 19 21.9107904.188 mas-198.099 mas81.6645670.55117422DR 21-W-1.112 (3)5.1003.40045.000
+20 38 55.4148+42 19 26.74169144.39 mas4632.8 mas81.6666610.55064633DR 21-W-5.38 (3)8.3004.00079.000
+20 38 53.7069+42 19 11.6455-16474.6 mas-10463.3 mas81.6601330.55227444DR 21-W-2.110 (2)11.1006.20045.000
+20 38 54.294+42 19 21.6786-7668.35 mas-430.188 mas81.6634450.55253255DR 21-W-2.77 (2)5.8004.50066.000
+20 38 55.1025+42 19 29.82414460.16 mas7715.31 mas81.6667560.55193066DR 21-W-57 (2)7.3003.600152.000
+20 38 54.2762+42 19 16.5776-7934.27 mas-5531.24 mas81.6622870.55171477DR 21-W-3.36 (3)14.2006.100177.000
+20 38 53.4375+42 19 8.63037-20515.4 mas-13478.4 mas81.6589630.55242488DR 21-W-1.56 (3)3.8003.50055.000
+20 38 54.2421+42 19 3.57548-8446.95 mas-18533.3 mas81.6593550.54960299DR 21-W-58 (2)3.7002.600123.000
+20 38 54.4594+42 19 10.8878-5187.7 mas-11221 mas81.6613750.5503051010DR 21-W-4.59 (2)5.6004.100135.000
+20 38 55.7218+42 19 35.258913749.2 mas13150.1 mas81.6691150.5513341111DR 21-W-3.910 (4)3.6003.20096.000
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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 LIE97

    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 LIE97 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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