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BAR71 - Detection of Methyl Alcohol in Orion at a Wavelength of ~1 Centimeter

Short title: Barrett et al. (1971)
Authors: Barrett, A. H. Schwartz, P. R. Waters, J. W.
Journal: Astrophysical Journal, vol. 168, p.L101
Bibcode: 1971ApJ...168L.101B

PDF: BAR71.pdf

Detection table from Barrett et al. (1971)

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ID Obs. RA Obs. Dec l b Group id Source name Line Ta Telescope Beam Detection Date
(J2000) (J2000) (deg.) (deg.) CH3OH (class I) (K) (arcsec) Yes/No
105 35 15.5-05 22 26.6208.9940-19.3806G208.993-19.385
Orion24.933 GHz (I)
1.0 (0.2)HAYS78+H2O +CH3OH I +CH3OH II +OH +SiO April-May 1971
205 35 15.5-05 22 26.6208.9940-19.3806G208.993-19.385
Orion24.959 GHz (I)
1.1 (0.2)HAYS78+H2O +CH3OH I +CH3OH II +OH +SiO April-May 1971
305 35 15.5-05 22 26.6208.9940-19.3806G208.993-19.385
Orion25.0 GHz (I)
1.7 (0.2)HAYS78+H2O +CH3OH I +CH3OH II +OH +SiO April-May 1971
405 35 15.5-05 22 26.6208.9940-19.3806G208.993-19.385
Orion25.1 GHz (I)
1.5 (0.2)HAYS78+H2O +CH3OH I +CH3OH II +OH +SiO April-May 1971
505 35 15.5-05 22 26.6208.9940-19.3806G208.993-19.385
Orion25.2 GHz (I)
0.7 (0.2)HAYS78+H2O +CH3OH I +CH3OH II +OH +SiO April-May 1971
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Non-detection table from Barrett et al. (1971)

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ID Obs. RA Obs. Dec l b Group id Source name Line Telescope RMS Beam Detection Date
(J2000) (J2000) (deg.) (deg.) CH3OH (class I) (K) (arcsec) Yes/No
102 09 26.1+76 09 19127.653914.0037G127.654+14.004
Cloud 127.725.1 GHz (I)
HAYS1.00078-CH3OH I April-May 1971
202 25 38.4+62 05 43.2133.71181.2115G133.715+1.215
W325.1 GHz (I)
HAYS2.00078+H2O -CH3OH I +CH3OH II +OH April-May 1971
302 27 4.4+61 52 21.6133.94871.0638G133.948+1.064
W3 OH25.1 GHz (I)
HAYS1.00078+H2O +CH3OH I +CH3OH II +OH April-May 1971
404 41 35.5+25 24 5.5174.5895-13.6451G174.590-13.645
Cloud 225.1 GHz (I)
HAYS1.00078-CH3OH I April-May 1971
505 11 19.7+52 52 27.7156.43957.8347G156.438+7.835
IRC 5013725.1 GHz (I)
HAYS1.00078+H2O -CH3OH I +OH +SiO April-May 1971
607 22 56.6-25 46 14.6239.3524-5.0727G239.353-5.065
VY CMa25.1 GHz (I)
HAYS0.80078+H2O -CH3OH I -CH3OH II +OH +SiO April-May 1971
709 48 0.5+13 16 38.7221.455945.0711G221.445+45.057
IRC+1021625.1 GHz (I)
HAYS1.00078+H2O -CH3OH I -OH April-May 1971
810 16 3.3+30 34 26197.711655.9682G197.715+55.964
CIT-625.1 GHz (I)
HAYS1.00078+H2O -CH3OH I -OH +SiO April-May 1971
914 24 12.9+25 42 2134.285369.2084G34.278+69.213
RX Boo25.1 GHz (I)
HAYS0.80078+H2O -CH3OH I +OH +SiO April-May 1971
1017 45 38.7-28 59 39.7359.9532-0.0350G359.985-0.050
Sgr A25.1 GHz (I)
HAYS0.60078+H2O +CH3OH I +CH3OH II +OH +SiO April-May 1971
1117 47 20.9-28 24 50.20.6431-0.0525G0.667-0.036
Sgr B225.1 GHz (I)
HAYS0.40078+H2O +CH3OH I +CH3OH II +OH +SiO April-May 1971
1217 47 20.8-28 23 32.20.6615-0.0412G0.667-0.036
25.1 GHz (I)
HAYS0.60078+H2O +CH3OH I +CH3OH II +OH +SiO April-May 1971
1319 06 22.6+08 13 47.241.95280.4527G41.952+0.454
R Aql25.1 GHz (I)
HAYS1.00078+H2O -CH3OH I +OH +SiO April-May 1971
1419 10 13.6+09 06 17.443.16790.0110G43.166+0.011
W49 (N)25.1 GHz (I)
HAYS0.80078+H2O +CH3OH I +CH3OH II +OH April-May 1971
1519 23 44.7+14 30 23.549.4885-0.3916G49.488-0.387
W5125.1 GHz (I)
HAYS0.80078+H2O +CH3OH I +CH3OH II +OH -SiO April-May 1971
1620 46 25.7+40 06 56.480.7980-1.9219G80.798-1.921
NML Cyg25.1 GHz (I)
HAYS1.00078+H2O -CH3OH I +OH +SiO April-May 1971
1722 36 51.1+75 14 3.9114.541014.6017G114.541+14.602
Cloud 11425.1 GHz (I)
HAYS1.00078-CH3OH I April-May 1971
1823 23 27.8+58 49 8.5111.7438-2.1285G111.747-2.110
Cas A25.1 GHz (I)
HAYS1.00078-CH3OH I -CH3OH II April-May 1971
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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 BAR71

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    Longitude-Velocity Map is taken form Dame, Hartmann & Thaddeus (2001)

  • Distribution of sources from BAR71 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