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PAL93C - Water masers associated with Herbig Ae/Be stars.

Short title: Palla & Prusti (1993)
Authors: Palla, F.Prusti, T.
Journal: Astronomy and Astrophysics, Vol. 272, p. 249-254 (1993)
Bibcode: 1993A&A...272..249P

Detection table from Palla & Prusti (1993)

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ID Obs. RA Obs. Dec l b Group id Source name Line Vrange Vpeak FWHM Fpeak ∫F dv Telescope Vstep RMS Beam Detection Class Dist. (parallax) Date
(J2000) (J2000) (deg.) (deg.) H2O (km/s) (km/s) (km/s) (Jy) (Jy*km/s) (km/s) (Jy) (arcsec) Yes/No (kpc)
120 20 28.4+41 21 51.378.87212.7696G78.871+2.762
BD+40°412422 GHz; -87;-65-760.1641.824.3MED0.331.500114+H2O +CH3OH I -CH3OH II -SiO SFR_MIXED24/04/90
20 20 28.4+41 21 51.378.87212.7696G78.871+2.762
BD+40°412422 GHz; -66;-88-83.60.6583.230.4MED0.331.500114+H2O +CH3OH I -CH3OH II -SiO SFR_MIXED23/07/90
20 20 28.4+41 21 51.378.87212.7696G78.871+2.762
BD+40°412422 GHz; -66;-82-72.70.16456.1225.2MED0.331.500114+H2O +CH3OH I -CH3OH II -SiO SFR_MIXED24/10/90
20 20 28.4+41 21 51.378.87212.7696G78.871+2.762
BD+40°412422 GHz; -61;-96-71.30.3298.493MED0.331.500114+H2O +CH3OH I -CH3OH II -SiO SFR_MIXED30/01/91
20 20 28.4+41 21 51.378.87212.7696G78.871+2.762
BD+40°412422 GHz; -68;-84-800.0829.760.1MED0.331.500114+H2O +CH3OH I -CH3OH II -SiO SFR_MIXED21/05/91
20 20 28.4+41 21 51.378.87212.7696G78.871+2.762
BD+40°412422 GHz; 26;2927.10.0827.68MED0.331.500114+H2O +CH3OH I -CH3OH II -SiO SFR_MIXED21/01/91
20 20 28.4+41 21 51.378.87212.7696G78.871+2.762
BD+40°412422 GHz; 26;2827.10.0828.29.2MED0.331.500114+H2O +CH3OH I -CH3OH II -SiO SFR_MIXED23/05/91
821 39 58.2+50 14 20.594.6024-1.7962G94.603-1.796
V645 Cyg22 GHz; -43;-50-460.16453.793.2MED0.331.500114+H2O -CH3OH I +CH3OH II -OH -SiO SFR_MIXED29/01/89
21 39 58.2+50 14 20.594.6024-1.7962G94.603-1.796
V645 Cyg22 GHz; -49;-46-47.50.6582.8MED0.331.500114+H2O -CH3OH I +CH3OH II -OH -SiO SFR_MIXED25/04/90
21 39 58.2+50 14 20.594.6024-1.7962G94.603-1.796
V645 Cyg22 GHz; -44.60.6589.6MED0.331.500114+H2O -CH3OH I +CH3OH II -OH -SiO SFR_MIXED04/02/90
21 39 58.2+50 14 20.594.6024-1.7962G94.603-1.796
V645 Cyg22 GHz; -46.143.5MED0.331.500114+H2O -CH3OH I +CH3OH II -OH -SiO SFR_MIXED1979
1221 43 2.3+66 06 28.9105.40509.8774G105.405+9.877
LkHa 23422 GHz; -22.1;-10.8-20.70.082231.8247.8MED0.331.500114+H2O -CH3OH I -CH3OH II SFR_MIXED02/04/90
21 43 2.3+66 06 28.9105.40509.8774G105.405+9.877
LkHa 23422 GHz; -24;-9-220.329119152MED0.331.500114+H2O -CH3OH I -CH3OH II SFR_MIXED24/10/90
21 43 2.3+66 06 28.9105.40509.8774G105.405+9.877
LkHa 23422 GHz; -7.80.658267.6MED0.331.500114+H2O -CH3OH I -CH3OH II SFR_MIXED10/02/90
21 43 2.3+66 06 28.9105.40509.8774G105.405+9.877
LkHa 23422 GHz; -8.343.1MED0.331.500114+H2O -CH3OH I -CH3OH II SFR_MIXED10/78
21 43 2.3+66 06 28.9105.40509.8774G105.405+9.877
LkHa 23422 GHz; -9.740MED0.331.500114+H2O -CH3OH I -CH3OH II SFR_MIXED02/79
21 43 2.3+66 06 28.9105.40509.8774G105.405+9.877
LkHa 23422 GHz; -1939.3MED0.331.500114+H2O -CH3OH I -CH3OH II SFR_MIXED29/09/85
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Non-detection table from Palla & Prusti (1993)

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ID Obs. RA Obs. Dec l b Group id Source name Line Fpeak Telescope Vstep RMS Beam Detection Class Date
(J2000) (J2000) (deg.) (deg.) H2O (Jy) (km/s) (Jy) (arcsec) Yes/No
120 20 28.4+41 21 51.378.87212.7696G78.871+2.762
BD+40°412422 GHz; <5.2MED0.331.500114+H2O +CH3OH I -CH3OH II -SiO SFR_MIXED18/02/90
221 39 58.2+50 14 20.594.6024-1.7962G94.603-1.796
V645 Cyg22 GHz; <2.3MED0.331.500114+H2O -CH3OH I +CH3OH II -OH -SiO SFR_MIXED17/07/90
21 39 58.2+50 14 20.594.6024-1.7962G94.603-1.796
V645 Cyg22 GHz; <8.5MED0.331.500114+H2O -CH3OH I +CH3OH II -OH -SiO SFR_MIXED24/10/90
400 11 26+58 49 47117.7644-3.6401G117.766-3.639
LkHa 19822 GHz; MED0.331.420114+H2O -CH3OH I -CH3OH II -OH SFR_MIXED2
500 43 18.3+61 54 40.3121.9745-0.9454G121.975-0.946
BD+61°15422 GHz; MED0.331.210114-H2O -CH3OH I EVOLVED2
602 16 30.2+55 22 56.6134.8789-5.5038G134.879-5.504
RNO622 GHz; MED0.331.190114-H2O -CH3OH I SFR_MIXED4
703 49 36.1+38 58 55156.7959-11.9028G156.797-11.902
XY Per A+B22 GHz; MED0.331.080114-H2O -CH3OH I EVOLVED2
804 18 40.6+28 19 15.9168.8355-15.5494G168.835-15.549
Elias 122 GHz; MED0.330.980114-H2O -CH3OH I -OH EVOLVED2
904 37 30.5+24 20 45.2174.8201-15.0315G174.820-15.032
BD+24°67622 GHz; MED0.331.270114-H2O 4
1004 55 45.7+30 33 5.9172.4984-7.9809G172.498-7.982
AB Aur22 GHz; MED0.331.350114-H2O -CH3OH I -CH3OH II -SiO SFR_MIXED2
1105 11 36.4-02 22 48.5203.2050-23.2126G203.205-23.212
V1012 0ri22 GHz; MED0.332.000114-H2O -CH3OH I -OH SFR4
1205 31 28.1+12 09 10.5192.6353-11.6229G192.635-11.623
HK Ori22 GHz; MED0.331.400114-H2O -CH3OH I -SiO EVOLVED2
1305 35 9.6+10 01 51.4194.9696-11.9411G194.970-11.941
BD+9°88022 GHz; MED0.331.150114-H2O -CH3OH I EVOLVED2
1405 35 50.4-05 28 35.2209.1601-19.2979G209.160-19.298
T Ori22 GHz; MED0.332.340114-H2O -CH3OH I EVOLVED3
1505 36 25.4-06 42 56.7210.4043-19.7242G210.404-19.724
V380 Ori22 GHz; MED0.331.300114-H2O -CH3OH I -CH3OH II SFR_MIXED1
1605 37 13.3-06 35 0.2210.3722-19.4879G210.372-19.488
BF Ori22 GHz; MED0.331.490114-H2O EVOLVED2
1705 38 14.5-05 24 48.6209.3864-18.7359G209.393-18.739
HD 3741122 GHz; MED0.331.510114-H2O -CH3OH I EVOLVED2
1805 39 30.1+26 22 26.3181.4663-2.5003G181.467-2.499
RR Tau22 GHz; MED0.331.320114-H2O -CH3OH I EVOLVED2
1905 39 31.5+04 06 35.2200.7873-13.9641G200.787-13.964
HD 3749022 GHz; MED0.331.410114-H2O 3
2006 01 58.4+16 30 54.7192.6213-3.0444G192.623-3.040
HD 25055022 GHz; MED0.331.390114+H2O -CH3OH I -OH SFR_MIXED2
2106 07 49.5+18 39 27.2191.4339-0.7805G191.434-0.780
LkHa 20822 GHz; MED0.331.340114+H2O EVOLVED2
2206 18 44.9+15 16 43.4195.6511-0.1081G195.651-0.108
MWC 13722 GHz; MED0.331.280114-H2O -CH3OH I -CH3OH II SFR_MIXED3
2306 31 9.2+10 26 10.2201.34490.2995G201.342+0.291
VY Mon22 GHz; MED0.331.260114-H2O -CH3OH I -CH3OH II -SiO SFR_MIXED4
2406 32 40.9+10 09 33.6201.76430.5051G201.765+0.507
LkHa 21522 GHz; MED0.331.050114-H2O -CH3OH I -CH3OH II EVOLVED1
2506 33 4.4+10 19 20.9201.66400.6659G201.664+0.666
HD 25943122 GHz; MED0.331.060114-H2O -CH3OH II SFR_MIXED2
2606 39 10+08 44 10.5203.76351.2709G203.763+1.271
R Mon22 GHz; MED0.331.360114-H2O -CH3OH I -CH3OH II -OH EVOLVED2
2706 40 44.6+09 48 1.7202.99482.1038G202.995+2.104
LkHa 2522 GHz; MED0.331.450114-H2O -CH3OH I -OH SFR_MIXED2
2807 01 44.9-11 17 21.8224.1522-2.8668G224.152-2.867
HD 5272122 GHz; MED0.332.140114-H2O 3
2907 02 42.6-11 26 11.9224.3911-2.7240G224.391-2.725
LkHa21822 GHz; MED0.331.720114-H2O -CH3OH I EVOLVED3
3007 03 43.2-11 33 6.1224.6066-2.5564G224.607-2.557
Z CMa22 GHz; MED0.331.330114+H2O -CH3OH I -CH3OH II -OH SFR_MIXED3
3107 04 6.9-11 26 6.8224.5470-2.4173G224.547-2.418
LkHa 22022 GHz; MED0.331.440114-H2O -CH3OH I SFR_MIXED3
3207 04 21.9-10 26 32.8223.6918-1.9084G223.706-1.901
HD 5336722 GHz; MED0.331.310114-H2O -CH3OH I EVOLVED3
3316 40 13.4-23 52 48.1355.600014.8504G355.600+14.850
HD 15019322 GHz; MED0.332.060114-H2O 3
3417 10 08-27 15 19.1357.06407.4477G357.064+7.448
KK Oph22 GHz; MED0.332.150114-H2O -CH3OH I +SiO EVOLVED3
3517 56 18.6-21 56 22.77.24601.5069G7.246+1.507
HD 16329622 GHz; MED0.332.330114-H2O EVOLVED3
3618 05 49.7-24 15 19.26.3189-1.5416G6.319-1.542
LkHa 11822 GHz; MED0.331.570114-H2O EVOLVED5 .
3718 27 40.5-03 51 2126.78163.5112G26.782+3.511
MWC 29722 GHz; MED0.331.560114-H2O SFR3
3818 28 47.9+00 08 39.130.47325.1014G30.473+5.101
VV Ser22 GHz; MED0.331.510114+H2O -CH3OH I EVOLVED2
3918 29 22.8-06 03 57.725.01612.1126G25.012+2.097
MWC 30022 GHz; MED0.331.330114-H2O -CH3OH I -CH3OH II -OH -SiO EVOLVED3
4018 33 21.3-04 58 6.426.44721.7419G26.448+1.743
AS 31022 GHz; MED0.331.620114-H2O -CH3OH I -CH3OH II SFR_MIXED5
4119 25 58.7+21 12 30.855.64432.3146G55.645+2.314
WW Vul22 GHz; MED0.331.490114-H2O -CH3OH I EVOLVED4
4219 29 0.8+09 38 38.745.8155-3.8315G45.817-3.832
Par 21 .22 GHz; MED0.331.840114-H2O -CH3OH I EVOLVED4
4320 24 16.4+42 17 46.980.04272.7190G80.045+2.723
BD+41°373122 GHz; MED0.331.080114-H2O -CH3OH I EVOLVED2
4420 45 54+67 57 38.8102.969815.2315G102.970+15.231
PV Cep22 GHz; MED0.331.380114+H2O -CH3OH I -CH3OH II -OH EVOLVED2
4520 47 23.4+43 44 39.783.73930.2115G83.739+0.212
V517 Cyg22 GHz; MED0.331.110114-H2O -CH3OH I EVOLVED6
4620 47 37.5+43 47 25.483.80170.2075G83.802+0.207
AS 44222 GHz; MED0.331.100114-H2O -CH3OH I SFR_MIXED2
4720 58 53.7+44 15 28.485.4598-1.0469G85.460-1.047
V1057 Cyg22 GHz; MED0.331.210114+H2O -CH3OH I -CH3OH II -SiO SFR_MIXED5
4821 01 36.9+68 09 47.6104.061514.1925G104.062+14.193
HD 20077522 GHz; MED0.331.000114-H2O -CH3OH I -CH3OH II SFR_MIXED3
4921 52 34.1+47 13 43.994.2490-5.4356G94.250-5.436
BD+46°347122 GHz; MED0.331.570114-H2O -CH3OH I -CH3OH II SFR_MIXED2
5021 54 18.9+47 12 10.994.4650-5.6416G94.465-5.642
LkHa 25722 GHz; MED0.331.200114-H2O -CH3OH I EVOLVED5
5122 34 41+40 40 3.796.7291-15.1444G96.729-15.144
LkHa 23322 GHz; MED0.331.300114-H2O -CH3OH I GALAXY2
5222 53 15.2+62 07 58.6109.59402.3614G109.600+2.373
HD 21662922 GHz; MED0.331.310114-H2O -CH3OH I EVOLVED2
5323 17 25.8+60 50 44.9111.72980.0352G111.730+0.035
MWC 108022 GHz; MED0.331.080114-H2O -CH3OH I -CH3OH II SFR_MIXED1
5423 58 41.5+66 26 11.9117.68604.1036G117.686+4.104
MacC H422 GHz; MED0.331.370114+H2O -CH3OH I EVOLVED4
×
  • 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 PAL93C

    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 PAL93C 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