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LEW93 - A Search for Water and Mainline OH Masers from OH / Infrared Star Colour Mimics

Short title: Lewis & Engels (1993)
Authors: Lewis, B. M. Engels, D.
Journal: Monthly Notices of the Royal Astronomical Society, Vol. 265, NO. 1/NOV1, P. 161, 1993
Bibcode: 1993MNRAS.265..161L

Detection table from Lewis & Engels (1993)

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ID Obs. RA Obs. Dec l b Group id Source name Frequency Vrange Vpeak Fpeak List Detection Class Dist. (parallax) Ref.
(J2000) (J2000) (deg.) (deg.) (MHz) (km/s) (km/s) (Jy) Yes/No (kpc)
120 12 57.6+33 30 2571.5210-0.3847G71.522-0.385
IRAS 20110+332116672.27.40.352ENG15+H2O +CH3OH I +CH3OH II +OH SFRLEW93
219 51 29.7+27 08 5363.67630.1663G63.676+0.166
IRAS 19494+2701166743.74.90.020ENG15+OH EVOLVEDLEW93
319 42 03+23 06 0259.1032-0.0237G59.103-0.024
IRAS 19399+225816672.06.30.100ENG15-H2O +OH +SiO UNKLEW93
419 37 20.5+19 28 5255.4129-0.8516G55.413-0.852
IRAS 19351+192216673.152.80.013ENG15-H2O +OH -SiO EVOLVEDLEW93
19 37 20.5+19 28 5255.4129-0.8516G55.413-0.852
IRAS 19351+192216653.152.80.033ENG15-H2O +OH -SiO EVOLVEDLEW93
619 25 50.5+36 21 3069.12039.3889G69.120+9.389
IRAS 19240+3615166729.720.10.012ENG15-H2O +OH +SiO EVOLVEDLEW93
719 22 25.4+20 15 3354.41392.5995G54.414+2.599
IRAS 19202+200916678.68.60.020ENG15+OH -SiO EVOLVEDLEW93
19 22 25.4+20 15 3354.41392.5995G54.414+2.599
IRAS 19202+200916658.68.60.021ENG15+OH -SiO EVOLVEDLEW93
919 12 44.9+09 41 0543.9697-0.2721G43.970-0.272
IRAS 19103+0935166750.516.60.015ENG15+OH SFR_MIXEDLEW93
19 12 44.9+09 41 0543.9697-0.2721G43.970-0.272
IRAS 19103+0935166528.115.70.035ENG15+OH SFR_MIXEDLEW93
1119 07 59.2+07 56 4641.8844-0.0318G41.884-0.032
IRAS 19055+0751166722.64.60.011ENG15-CH3OH II +OH EVOLVEDLEW93
19 07 59.2+07 56 4641.8844-0.0318G41.884-0.032
IRAS 19055+075116651.516.90.027ENG15-CH3OH II +OH EVOLVEDLEW93
1318 53 53.6+02 39 0135.57050.6623G35.571+0.662
IRAS 18513+023516674.277.50.027ENG15-H2O +OH EVOLVEDLEW93
1405 37 47.8+31 59 24176.51670.1819G176.517+0.182
IRAS 05345+3157166718.4-18.40.038ENG15+H2O -CH3OH I -CH3OH II +OH -SiO SFR_MIXEDLEW93
05 37 47.8+31 59 24176.51670.1819G176.517+0.182
IRAS 05345+3157166519.1-18.40.012ENG15+H2O -CH3OH I -CH3OH II +OH -SiO SFR_MIXEDLEW93
1620 38 57.7+12 05 3356.9170-17.3342G56.917-17.334
IRAS 20365+1154166718.218.20.079ENG15-H2O -CH3OH II +OH EVOLVEDLEW93
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Non-detection table from Lewis & Engels (1993)

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ID Obs. RA Obs. Dec l b Group id Source name Line Fpeak List Detection Class Ref.
(J2000) (J2000) (deg.) (deg.) OH (Jy) Yes/No
120 12 57.6+33 30 2571.5210-0.3847G71.522-0.385
IRAS 20110+33211.665 GHz; 0.030ENG15+H2O +CH3OH I +CH3OH II +OH SFRLEW93
220 00 29.6+36 46 0972.89943.5185G72.899+3.519
IRAS 19586+36371.667 GHz; 0.030ENG15-H2O -CH3OH II -OH +SiO EVOLVEDLEW93
320 00 29.6+36 46 0972.89943.5185G72.899+3.519
IRAS 19586+36371.665 GHz; 0.030ENG15-H2O -CH3OH II -OH +SiO EVOLVEDLEW93
419 59 15.7+31 52 0968.59041.1646G68.590+1.165
IRAS 19573+31431.665 GHz; 0.030ENG15-OH -SiO UNKLEW93
519 59 15.7+31 52 0968.59041.1646G68.590+1.165
IRAS 19573+31431.667 GHz; 0.030ENG15-OH -SiO UNKLEW93
620 00 30.9+27 00 3764.6001-1.6217G64.600-1.622
IRAS 19584+26521.665 GHz; 0.030ENG15-CH3OH II -OH -SiO EVOLVEDLEW93
720 00 30.9+27 00 3764.6001-1.6217G64.600-1.622
IRAS 19584+26521.667 GHz; 0.030ENG15-CH3OH II -OH -SiO EVOLVEDLEW93
819 57 48.2+33 41 2069.98232.3770G69.982+2.377
IRAS 19558+33331.667 GHz; 0.030ENG15-CH3OH II -OH -SiO EVOLVEDLEW93
919 57 48.2+33 41 2069.98232.3770G69.982+2.377
IRAS 19558+33331.665 GHz; 0.030ENG15-CH3OH II -OH -SiO EVOLVEDLEW93
1019 56 47.8+30 43 5867.34611.0202G67.346+1.020
IRAS 19548+30351.667 GHz; 0.030ENG15-OH EVOLVEDLEW93
1119 56 47.8+30 43 5867.34611.0202G67.346+1.020
IRAS 19548+30351.665 GHz; 0.030ENG15-OH EVOLVEDLEW93
1219 51 29.7+27 08 5363.67630.1663G63.676+0.166
IRAS 19494+27011.665 GHz; 0.030ENG15+OH EVOLVEDLEW93
1319 48 38.1+27 59 3264.08101.1413G64.081+1.141
IRAS 19466+27511.667 GHz; 0.030ENG15+H2O -CH3OH II +OH -SiO EVOLVEDLEW93
1419 48 38.1+27 59 3264.08101.1413G64.081+1.141
IRAS 19466+27511.665 GHz; 0.030ENG15+H2O -CH3OH II +OH -SiO EVOLVEDLEW93
1519 43 55.6+33 25 2368.28374.7337G68.284+4.734
IRAS 19420+33181.667 GHz; 0.030ENG15-OH EVOLVEDLEW93
1619 43 55.6+33 25 2368.28374.7337G68.284+4.734
IRAS 19420+33181.665 GHz; 0.030ENG15-OH EVOLVEDLEW93
1719 42 03+23 06 0259.1032-0.0237G59.103-0.024
IRAS 19399+22581.665 GHz; 0.030ENG15-H2O +OH +SiO UNKLEW93
1819 33 16.7+17 52 0353.5348-0.7954G53.535-0.795
IRAS 19310+17451.667 GHz; 0.030ENG15-H2O -CH3OH I -OH -SiO SFRLEW93
1919 33 16.7+17 52 0353.5348-0.7954G53.535-0.795
IRAS 19310+17451.665 GHz; 0.030ENG15-H2O -CH3OH I -OH -SiO SFRLEW93
2019 30 19.6+22 59 5957.70062.2821G57.701+2.282
IRAS 19282+22531.667 GHz; 0.030ENG15-OH -SiO EVOLVEDLEW93
2119 30 19.6+22 59 5957.70062.2821G57.701+2.282
IRAS 19282+22531.665 GHz; 0.030ENG15-OH -SiO EVOLVEDLEW93
2219 25 50.5+36 21 3069.12039.3889G69.120+9.389
IRAS 19240+36151.665 GHz; 0.030ENG15-H2O +OH +SiO EVOLVEDLEW93
2319 25 0.1+17 06 5451.92930.5770G51.929+0.577
IRAS 19227+17001.667 GHz; 0.030ENG15-H2O +OH -SiO EVOLVEDLEW93
2419 25 0.1+17 06 5451.92930.5770G51.929+0.577
IRAS 19227+17001.665 GHz; 0.030ENG15-H2O +OH -SiO EVOLVEDLEW93
2519 15 53.6+09 36 5344.2677-0.9911G44.268-0.991
IRAS 19135+09311.667 GHz; 0.030ENG15-H2O -OH -SiO EVOLVEDLEW93
2619 15 53.6+09 36 5344.2677-0.9911G44.268-0.991
IRAS 19135+09311.665 GHz; 0.030ENG15-H2O -OH -SiO EVOLVEDLEW93
2719 01 10.5+01 11 1635.0998-1.6240G35.100-1.624
IRAS 18586+01061.667 GHz; 0.030ENG15-H2O -CH3OH I -CH3OH II -OH SFRLEW93
2819 01 10.5+01 11 1635.0998-1.6240G35.100-1.624
IRAS 18586+01061.665 GHz; 0.030ENG15-H2O -CH3OH I -CH3OH II -OH SFRLEW93
2907 01 8.4+15 03 40200.50328.9086G200.503+8.909
IRAS 06582+15071.667 GHz; 0.030ENG15-CH3OH II -OH -SiO EVOLVEDLEW93
3018 30 15.9+21 51 5750.491414.2422G50.492+14.242
IRAS 18281+21491.665 GHz; 0.030ENG15-H2O -OH -SiO EVOLVEDLEW93
3118 30 15.9+21 51 5750.491414.2422G50.492+14.242
IRAS 18281+21491.667 GHz; 0.030ENG15-H2O -OH -SiO EVOLVEDLEW93
3218 53 53.6+02 39 0135.57050.6623G35.571+0.662
IRAS 18513+02351.665 GHz; 0.030ENG15-H2O +OH EVOLVEDLEW93
3307 01 8.4+15 03 40200.50328.9086G200.503+8.909
IRAS 06582+15071.665 GHz; 0.030ENG15-CH3OH II -OH -SiO EVOLVEDLEW93
3406 20 45.8+04 05 11205.7757-4.9317G205.776-4.932
IRAS 06181+04061.667 GHz; 0.030ENG15-H2O -OH -SiO EVOLVEDLEW93
3506 20 45.8+04 05 11205.7757-4.9317G205.776-4.932
IRAS 06181+04061.665 GHz; 0.030ENG15-H2O -OH -SiO EVOLVEDLEW93
3620 23 40.3+33 40 3772.9160-2.1339G72.916-2.134
IRAS 20217+33301.665 GHz; 0.030ENG15-H2O -OH +SiO EVOLVEDLEW93
3720 23 40.3+33 40 3772.9160-2.1339G72.916-2.134
IRAS 20217+33301.667 GHz; 0.030ENG15-H2O -OH +SiO EVOLVEDLEW93
3820 24 1.1+34 14 3973.4222-1.8674G73.422-1.867
IRAS 20220+34041.665 GHz; 0.030ENG15-CH3OH II -OH +SiO EVOLVEDLEW93
3920 24 1.1+34 14 3973.4222-1.8674G73.422-1.867
IRAS 20220+34041.667 GHz; 0.030ENG15-CH3OH II -OH +SiO EVOLVEDLEW93
4020 38 57.7+12 05 3356.9170-17.3342G56.917-17.334
IRAS 20365+11541.665 GHz; 0.030ENG15-H2O -CH3OH II +OH EVOLVEDLEW93
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  • Distribution of sources in all sky (l,b)

    0

  • 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 LEW93

    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 LEW93 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

    Download UKIDSS K FITS
    2MASS K

    Download 2MASS K FITS