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GOM17 - A Search for Water Maser Emission from Brown Dwarfs and Low-luminosity Young Stellar Objects

Short title: Gomez et al. (2017)
Authors: Gomez, Jose F.Palau, AinaUscanga, LuceroManjarrez, GuillermoBarrado, David
Journal: The Astronomical Journal, Volume 153, Issue 5, article id. 221, 7 pp. (2017).
Bibcode: 2017AJ....153..221G

Detection table from Gomez et al. (2017)

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ID Obs. RA Obs. Dec l b Group id Source name Other name Image Line Vpeak Fpeak Telescope Vstep RMS Beam Detection Class Dist. (parallax) Date
(J2000) (J2000) (deg.) (deg.) Typea H2O (km/s) (Jy) (km/s) (Jy) (arcsec) Yes/No (kpc)
103 25 25.5+30 45 2.5158.0110-21.4361G158.000-21.441
L1448 IRS 2EFHC Image 22 GHz; 0.08 (0.03)-2.3EFF0.04716.00039+H2O -CH3OH II SFR2015 Sep 29
203 25 22.3+30 45 13.1157.9993-21.4404G158.000-21.441
L1448 IRS 2 Image 22 GHz; 0.46 (0.03)-1.19EFF0.0473.4 x 3.1+H2O -CH3OH II SFR2015 October 14
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Non-detection table from Gomez et al. (2017)

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ID Obs. RA Obs. Dec l b Group id Source name Other name Line Telescope Vstep RMS Beam Detection Class Date
(J2000) (J2000) (deg.) (deg.) Typea H2O (km/s) (Jy) (arcsec) Yes/No
103 25 10.2+30 23 55158.1892-21.7515G158.189-21.752
L1451-mmFHC22 GHz; EFF0.0470.02139-H2O SFR2015 Sep 29
203 25 25.5+30 45 2.5158.0110-21.4361G158.000-21.441
L1448 IRS 2E22 GHz; EFF0.0470.01439+H2O -CH3OH II SFR2015 Oct 03
303 29 25.4+31 28 15158.2821-20.3467G158.282-20.347
Per-Bolo 58FHC22 GHz; EFF0.0470.01839-H2O SFR_MIXED2015 Oct 01
403 33 21.2+31 07 35159.2153-20.1079G159.215-20.108
B1-b fieldbFHC22 GHz; EFF0.0470.01939-H2O -CH3OH II SFR2015 Sep 30
503 43 57.7+32 03 10.1160.4610-17.9691G160.461-17.969
IC 348-SMM2EBD-022 GHz; EFF0.0470.01839-H2O SFR2015 Sep 30
03 43 57.7+32 03 10.1160.4610-17.9691G160.461-17.969
IC 348-SMM2E22 GHz; EFF0.0470.02039-H2O SFR2015 Oct 03
703 44 10+32 04 5.4160.4856-17.9296G160.486-17.930
IC 348-173LL0-I22 GHz; EFF0.0470.01839-H2O SFR_MIXED2015 Oct 01
803 44 26.9+32 09 25160.4740-17.8232G160.474-17.823
IC 348-613BD-I22 GHz; EFF0.0470.01939-H2O SFR2015 Sep 30
903 44 29.5+32 00 53.2160.5773-17.9264G160.577-17.926
IC 348-205LLO-I22 GHz; EFF0.0470.01839-H2O SFR_MIXED2015 Oct 02
1003 44 30.8+32 02 42.9160.5603-17.9002G160.560-17.900
IC 348-382LLO-I22 GHz; EFF0.0470.02739-H2O SFR2015 Oct 03
1103 44 35.4+32 08 54.4160.5040-17.8104G160.501-17.802
IC 348-165LLO-I22 GHz; EFF0.0470.02639+H2O -CH3OH II SFR_MIXED2015 Oct 03
1204 17 26.4+27 39 20169.1423-16.2055G169.142-16.205
SSTB213 J041726.38+273920.0BD-I22 GHz; EFF0.0470.01839-H2O EVOLVED2015 Oct 01
1304 17 40.3+28 24 15.5168.6148-15.6523G168.615-15.652
SSTB213 J041740.32+282415.5BD-I22 GHz; EFF0.0470.01739-H2O EVOLVED2015 Oct 01
1404 17 57.8+27 41 05169.2032-16.1013G169.203-16.101
SSTB213 J041757.77+274105.5BD-I22 GHz; EFF0.0470.01739-H2O EVOLVED2015 Oct 01
1504 18 28.1+27 49 10.9169.1810-15.9274G169.181-15.927
SSTB213 J041828.08+274910.9BD-I22 GHz; EFF0.0470.01839-H2O SFR_MIXED2015 Oct 01
1604 18 36.3+27 14 42.2169.6381-16.2993G169.638-16.299
SSTB213 J041836.33+271442.2BD-I22 GHz; EFF0.0470.01839-H2O GALAXY2015 Oct 01
1704 18 47.8+27 40 55.3169.3372-15.9689G169.337-15.969
SSTB213 J041847.84+274055.3BD-I22 GHz; EFF0.0470.01739-H2O EVOLVED2015 Oct 01
1804 18 51.2+28 14 33.2168.9223-15.5752G168.922-15.575
KPNO-Tau 2BD-II22 GHz; EFF0.0470.01739-H2O EVOLVED2015 Oct 01
1904 18 58.1+28 12 23.5168.9678-15.5814G168.968-15.581
IRAS 04158+2805BD-I22 GHz; EFF0.0470.02139-H2O SFR2015 Sep 30
2004 19 13.1+27 47 26169.3214-15.8266G169.321-15.827
SSTB213 J041913.10+274726.0BD-I22 GHz; EFF0.0470.01639-H2O EVOLVED2015 Oct 01
2104 19 38.8+28 23 40.7168.9320-15.3439G168.932-15.344
SSTB213 J041938.77+282340.7BD-I22 GHz; EFF0.0470.01939-H2O EVOLVED2015 Oct 02
2204 19 42.5+27 13 40169.8258-16.1323G169.826-16.132
IRAS 04166+2706LLO-022 GHz; EFF0.0470.02739-H2O -CH3OH II SFR2015 Oct 02
2304 21 3.5+27 02 48.4170.1767-16.0355G170.177-16.035
L1521DLLO22 GHz; EFF0.0470.02839-H2O SFR2015 Oct 03
2404 20 19.2+28 06 10.3169.2579-15.4355G169.258-15.436
SSTB213 J042019.20+280610.3BD-I22 GHz; EFF0.0470.01839-H2O EVOLVED2015 Oct 02
2504 21 18.4+28 06 40.8169.4056-15.2707G169.406-15.271
SSTB213 J042118.43+280640.8BD-I22 GHz; EFF0.0470.01839-H2O EVOLVED2015 Oct 02
2604 21 56.9+15 29 45.9179.5563-23.5002G179.556-23.488
IRAM 04191+1522VeLLO-022 GHz; EFF0.0470.02039-H2O -CH3OH I -CH3OH II SFR2015 Sep 30
2704 27 57.3+26 19 18.1171.8095-15.3810G171.809-15.382
IRAS 04248+2612BD-I22 GHz; EFF0.0470.01939-H2O SFR2015 Sep 30
2804 28 39+26 51 35.1171.4992-14.9079G171.499-14.908
L1521F-IRSVeLLO-0/I22 GHz; EFF0.0470.01939-H2O SFR2015 Oct 02
2904 32 16+18 12 46178.9750-19.8695G178.975-19.869
MHO 5LLO-I22 GHz; EFF0.0470.01839-H2O EVOLVED2015 Sep 30
3004 35 35.4+24 08 19.5174.6941-15.5000G174.689-15.507
IRAS 04325+2402 A/BLLO-I22 GHz; EFF0.0470.01839+H2O -CH3OH II SFR2015 Oct 02
3104 38 14.9+26 11 39.9173.4669-13.7175G173.467-13.717
2MASS J04381486+2611399BD-II22 GHz; EFF0.0470.01739-H2O SFR2015 Sep 30
3204 39 04+25 44 26.4173.9467-13.8677G173.947-13.868
2MASS J04390396+2544264BD-II22 GHz; EFF0.0470.01939-H2O SFR2015 Sep 30
3304 39 47.3+26 01 39173.8269-13.5592G173.827-13.559
CFHT-BD-Tau 4LLO-II22 GHz; EFF0.0470.01939-H2O SFR_MIXED2015 Oct 02
3404 41 35.9+54 19 11.7152.55035.2664G152.550+5.266
L1415-IRSLLO-I22 GHz; EFF0.0470.01839-H2O EVOLVED2015 Oct 01
3504 41 48.2+25 34 30.5174.4829-13.4979G174.483-13.498
2MASS J04414825+2534304BD-II22 GHz; EFF0.0470.01939-H2O SFR2015 Sep 30
3604 42 38.6+29 43 55.3171.3328-10.6998G171.333-10.700
L1507ALLO22 GHz; EFF0.0470.01839-H2O SFR2015 Oct 02
3704 44 27.1+25 12 16.4175.1665-13.2684G175.167-13.268
2MASS J04442713 +2512164BD-II22 GHz; EFF0.0470.01939-H2O SFR2015 Sep 30
3804 52 6.7+30 47 17.5171.8184-8.4490G171.818-8.449
IRAS 04489+3042BD-I22 GHz; EFF0.0470.01739-H2O SFR2015 Oct 01
3918 16 16.9-02 32 3826.62576.6391G26.625+6.640
CB130-1 fieldcFHC22 GHz; EFF0.0470.02539-H2O -CH3OH II SFR2015 Sep 30
18 16 16.9-02 32 3826.62576.6391G26.625+6.640
CB130-1 fieldc22 GHz; EFF0.0470.02439-H2O -CH3OH II SFR2015 Oct 01
4118 17 0.4-18 01 5213.0299-0.8296G13.030-0.830
L328-IRSVeLLO-022 GHz; EFF0.0470.02439-H2O SFR2015 Sep 30
18 17 0.4-18 01 5213.0299-0.8296G13.030-0.830
L328-IRS22 GHz; EFF0.0470.01939-H2O SFR2015 Oct 01
4319 21 34.8+11 21 2346.4615-1.4119G46.461-1.412
L673-7-IRSVeLLO-022 GHz; EFF0.0470.01539-H2O SFR2015 Sep 29
4420 40 56.6+67 23 5.3102.200415.2809G102.200+15.281
L1148-IRSVeLLO-022 GHz; EFF0.0470.01439-H2O SFR2015 Sep 30
4521 24 7.5+49 59 0992.5682-0.2537G92.568-0.254
L1014-IRSVeLLO-I/II22 GHz; EFF0.0470.02139-H2O -CH3OH II SFR2015 Sep 30
21 24 7.5+49 59 0992.5682-0.2537G92.568-0.254
L1014-IRS22 GHz; EFF0.0470.01739-H2O -CH3OH II SFR2015 Oct 01
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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 GOM17

    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 GOM17 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