Display data from paper

Data: CH3OH_I

MCE16B - NH3(3,3) and CH3OH near Supernova Remnants: GBT and VLA Observations

  Interferometry data

Short title: McEwen et al. (2016b)
Authors: McEwen, Bridget C. Pihlström, Ylva M. Sjouwerman, Loránt O.
Journal: The Astrophysical Journal, Volume 826, Issue 2, article id. 189, 11 pp. (2016).
Bibcode: 2016ApJ...826..189M

PDF: MCE16B.pdf

Detection table from McEwen et al. (2016b)

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ID Obs. RA Obs. Dec RA offset Dec offset l b # Location Source name Other name Image Line Vpeak Fpeak ∫F dv Telescope Beam Date
(J2000) (J2000) (arcsec) (arcsec) (deg.) (deg.) Other Name CH3OH (class I) (km/s) (Jy/beam) (Jy/beam*km/s) (arcsec)
1+19 23 50+14 06 0049.140452-0.602805W51CG049.2-0.7 Image 36 GHz (I)
57.6 .. 76.20.13 .. 0.54 .. GBT2.65 x 1.92014 September 4
+19 22 42.69+14 09 55.5-1009.65235.549.069663-0.3321831B36-1W51C57.60.25
+19 22 42.21+14 09 51.5-1016.85231.549.067769-0.3309982B36-2W51C59.60.14
+19 22 42.76+14 10 02-1008.624249.071389-0.3315813B36-3W51C57.60.13
+19 22 41.42+14 09 3.5-1028.7183.549.054506-0.3344734B36-4W51C74.10.24
+19 22 25.7+14 06 35-1264.53548.988175-0.2979165F36-1W51C65.90.43
+19 22 26.01+14 06 36-1259.853648.989011-0.2988906F36-2W51C65.90.54
+19 22 26.11+14 06 37-1258.353748.989446-0.2991157F36-3W51C63.80.5
+19 22 12.08+14 02 49.5-1468.8-190.548.906984-0.2788968L36-1W51C67.90.43
+19 22 7.34+14 02 18.5-1539.9-221.548.890360-0.2660559L36-2W51C76.20.19
2+17 59 02-24 04 1.14255e-105.718211-0.100383G5.7-0.0- Image 36 GHz (I)
-26.40.21 .. 0.38 .. GBT2.65 x 1.92016 September 4
+17 58 44.99-24 08 38-255.149-277.9995.619011-0.0828331A36-1G5.7-0.0-26.40.38
+17 58 45.17-24 08 39.5-252.449-279.4995.618991-0.0836342A36-2G5.7-0.0-26.40.26
+17 58 44.85-24 08 36.5-257.249-276.4995.619106-0.0821643A36-3G5.7-0.0-26.40.21
3+17 59 02-24 04 1.14255e-105.718211-0.100383G5.7-0.0-44 GHz (I)
-24.40.35 .. 1.31 .. GBT2.11 x 1.842017 September 4
+17 58 44.48-24 08 37-262.799-276.9995.618284-0.0810141A44-1G5.7-0.0-24.41.31
+17 58 44.88-24 08 37-256.799-276.9995.619043-0.0823322A44-2G5.7-0.0-24.40.35
4+18 56 00+01 22 0034.668302-0.391577W44G034.7-0.4 Image 36 GHz (I)
40.9 .. 47.10.09 .. 0.3 .. GBT2.65 x 1.92018 September 4
+18 56 43.96+01 23 54.2659.4114.19934.780092-0.5400371A36-1W4440.90.25
+18 56 48.39+01 18 45.7725.85-194.30134.712260-0.5955652F36-1W4442.90.09
+18 56 50.82+01 18 17.3762.3-222.70134.709860-0.6081723G36-1W4442.90.14
+18 56 50.86+01 18 21.8762.9-218.20134.711049-0.6077504G36-2W4440.90.11
+18 56 52.49+01 18 12.3787.35-227.70134.711799-0.6149965G36-3W4447.10.12
+18 56 58.46+01 18 41.7876.9-198.30134.730416-0.6333966K36-1W44450.3
5+18 56 00+01 22 0034.668302-0.391577W44G034.7-0.444 GHz (I)
6.7 .. 56.90.21 .. 0.31 .. GBT2.11 x 1.842019 September 4
+18 56 49.86+01 18 43.2747.9-196.80134.714437-0.6013311K44-1W4456.90.21
+18 56 48.36+01 18 46.2725.4-193.80134.712327-0.5953912L44-1W44450.31
+18 56 57.86+01 17 27.7867.9-272.30134.710985-0.6405543P44-1W4435.60.26
+18 56 59.69+01 19 17.2895.35-162.80134.741530-0.6334554Q44-1W446.70.24
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Non-detection table from McEwen et al. (2016b)

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ID Obs. RA Obs. Dec l b Source name Other name Line Telescope Beam Date
(J2000) (J2000) (deg.) (deg.) Other Name CH3OH (class I) (arcsec)
1+19 23 50+14 06 0049.140452-0.602805W51CG049.2-0.744 GHz (I)
GBT2.11 x 1.842015 September 4
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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

    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 MCE16B

    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 MCE16B 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