Display data from paper

Data: CH3OH_I

MOM17 - The Zeeman Effect in the 44 GHz Class I Methanol Maser Line toward DR21(OH)

  Interferometry data

Short title: Momjian & Sarma (2017)
Authors: Momjian, E. Sarma, A. P.
Journal: The Astrophysical Journal, Volume 834, Issue 2, article id. 168, 6 pp. (2017).
Bibcode: 2017ApJ...834..168M

PDF: MOM17.pdf

Detection table from Momjian & Sarma (2017)

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ID Obs. RA Obs. Dec RA offset Dec offset l b Group id # Source name Line Vpeak Fpeak ∫F dv Telescope RMS Beam PA Detection
(J2000) (J2000) (arcsec) (arcsec) (deg.) (deg.) CH3OH (class I) (km/s) (Jy/beam) (Jy/beam*km/s) (mJy/beam) (arcsec) (deg.) Yes/No
1+20 39 08+42 22 4781.734390.553722G81.722+0.572
DR21(OH) 44 GHz (I)
0.203 .. 0.7860.35 .. 323.2 .. NRAOVLA12.0000.63 x 0.575.3+CH3OH I +CH3OH II +OH -SiO
+20 38 59.25+42 22 48.2-131.2491.200881.7182710.5753001DR21(OH)0.365 (0.002)219.23 (3.91)
+20 38 59.25+42 22 48.2-131.2491.200881.7182710.5753002DR21(OH)0.484 (0.010)82.74 (2.13)
+20 38 59.29+42 22 47-130.6490 mas81.7180810.5749993DR21(OH)0.372 (0.007)7.11 (0.12)
+20 38 59.31+42 22 49.1-130.3492.100881.7185810.5753054DR21(OH)0.352 (0.003)16.33 (0.12)
+20 38 59.33+42 22 46.8-130.049-0.199281.7181120.5748685DR21(OH)0.300 (0.008)6.64 (0.10)
+20 38 59.7+42 22 41.7-124.499-5.299281.7176800.5731026DR21(OH)0.786 (0.027)0.35 (0.01)
+20 38 59.71+42 22 45.3-124.349-1.699281.7184920.5736867DR21(OH)0.402 (0.034)0.52 (0.04)
+20 38 59.71+42 22 49.1-124.3492.100881.7193300.5743288DR21(OH)0.264 (0.041)1.03 (0.34)
+20 38 59.71+42 22 49.1-124.3492.100881.7193300.5743289DR21(OH)0.475 (0.148)0.49 (0.15)
+20 38 59.76+42 22 44.7-123.599-2.299281.7184540.57346210DR21(OH)0.365 (0.025)0.72 (0.04)
+20 38 59.85+42 22 45.4-122.249-1.599281.7187760.57336111DR21(OH)0.219 (0.003)14.79 (0.09)
+20 38 59.85+42 22 45.7-122.249-1.299281.7188430.57341112DR21(OH)0.227 (0.004)3.80 (0.04)
+20 38 59.89+42 22 44.9-121.649-2.099281.7187410.57317813DR21(OH)0.241 (0.004)16.46 (0.12)
+20 38 59.91+42 22 44.5-121.349-2.499281.7186900.57306214DR21(OH)0.203 (0.001)18.11 (0.14)
+20 38 59.96+42 22 34.7-120.599-12.299281.7166230.57128415DR21(OH)0.267 (0.021)0.75 (0.05)
+20 39 0.15+42 22 47.3-117.7490.300881.7197570.57294916DR21(OH)0.387 (0.003)10.48 (0.07)
+20 39 0.23+42 22 45.4-116.549-1.599281.7194880.57243217DR21(OH)0.309 (0.002)323.20 (1.22)
+20 39 0.23+42 22 45.4-116.549-1.599281.7194880.57243218DR21(OH)0.309 (0.011)44.30 (1.22)
+20 39 0.25+42 22 46.8-116.249-0.199281.7198340.57262019DR21(OH)0.279 (0.003)11.79 (0.10)
+20 39 0.25+42 22 46-116.249-0.999281.7196580.57248520DR21(OH)0.605 (0.041)0.83 (0.05)
+20 39 0.25+42 22 46-116.249-0.999281.7196580.57248521DR21(OH)0.368 (0.003)7.99 (0.06)
+20 39 0.3+42 22 46.6-115.499-0.399281.7198830.57246422DR21(OH)0.312 (0.007)0.90 (0.01)
+20 39 0.33+42 22 47.8-115.0490.800881.7202040.57259323DR21(OH)0.455 (0.004)1.15 (0.01)
+20 39 0.51+42 22 47.1-112.3490.100881.7203870.57203524DR21(OH)0.270 (0.018)0.72 (0.03)
+20 39 0.53+42 22 47.1-112.0490.100881.7204240.57198625DR21(OH)0.468 (0.023)1.82 (0.04)
+20 39 0.53+42 22 47.1-112.0490.100881.7204240.57198626DR21(OH)0.300 (0.054)1.09 (0.19)
+20 39 0.52+42 22 47.1-112.1990.100881.7204060.57201127DR21(OH)0.367 (0.022)2.77 (0.05)
+20 39 1.01+42 22 41.1-104.849-5.899281.7200000.56980028DR21(OH)0.470 (0.005)0.81 (0.01)
+20 39 1.2+42 22 40.5-101.999-6.499281.7202230.56923429DR21(OH)0.755 (0.031)0.63 (0.02)
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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

    Tip: Use "Box select" or "Lasso select" to display colour-selected sources in Aladin all-sky view

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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 MOM17

    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 MOM17 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