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Data: H2O, CH3OH_I

LYO14 - Unbiased Water and Methanol Maser Surveys of NGC 1333

Short title: Lyo et al. (2014)
Authors: Lyo, A.-Ran Kim, Jongsoo Byun, Do-Young Lee, Ho-Gyu
Journal: The Astronomical Journal, Volume 148, Issue 5, article id. 80, 10 pp. (2014).
Bibcode: 2014AJ....148...80L      BiBTeX

PDF: LYO14.pdf

Detection table from Lyo et al. (2014)

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ID Obs. RA Obs. Dec l b Source name Image Line Vpeak FWHM Fpeak ∫F dv Telescope Beam Date
(J2000) (J2000) (deg.) (deg.) CH3OH (class I) (km/s) (km/s) (Jy) (Jy*km/s) (arcsec)
103 29 9.7+31 13 21.6158.3945-20.5783NGC 1333 IRAS4A2 Image 44 GHz (I)
4.52 (0.29)9.42 (0.58)1.0910.89 (0.63)KVN622012 Mar 11
203 29 9.7+31 13 21.6158.3945-20.5783NGC 1333 IRAS4A244 GHz (I)
6.79 (0.04)1.54 (0.12)2.694.41 (0.35)KVN622012 Mar 11
303 29 9.7+31 13 21.6158.3945-20.5783NGC 1333 IRAS4A295 GHz (I)
5.28 (0.16)7.90 (0.49)2.4920.95 (0.82)KVN322012 Mar 11
403 29 9.7+31 13 21.6158.3945-20.5783NGC 1333 IRAS4A295 GHz (I)
7.08 (0.02)0.62 (0.11)5.733.80 (0.46)KVN322012 Mar 11
503 29 9.7+31 13 21.6158.3945-20.5783NGC 1333 IRAS4A2132.8 GHz (I)
3.98 (0.33)9.38 (0.63)2.9729.68 (2.02)KVN232012 Mar 11
603 29 9.7+31 13 21.6158.3945-20.5783NGC 1333 IRAS4A2132.8 GHz (I)
6.69 (0.08)2.32 (0.33)3.187.85 (1.44)KVN232012 Mar 11
703 29 11.7+31 13 7.8158.4031-20.5770NGC 1333 IRAS4B44 GHz (I)
4.84 (0.46)10.39 (1.07)0.77.79 (0.72)KVN622012 Apr 26
803 29 11.7+31 13 7.8158.4031-20.5770NGC 1333 IRAS4B44 GHz (I)
6.67 (0.07)1.82 (0.18)2.043.96 (0.44)KVN622012 Apr 26
903 29 11.7+31 13 7.8158.4031-20.5770NGC 1333 IRAS4B95 GHz (I)
6.66 (0.59)24.57 (10.69)0.287.36 (2.17)KVN322012 Apr 26
1003 29 11.7+31 13 7.8158.4031-20.5770NGC 1333 IRAS4B95 GHz (I)
7.17 (0.13)3.06 (0.32)2.227.23 (0.86)KVN322012 Apr 26
1103 29 11.7+31 13 7.8158.4031-20.5770NGC 1333 IRAS4B132.8 GHz (I)
5.45 (0.71)14.90 (1.37)0.9515.00 (1.55)KVN232012 Apr 26
1203 29 11.7+31 13 7.8158.4031-20.5770NGC 1333 IRAS4B132.8 GHz (I)
7.69 (0.05)3.16 (0.15)5.4418.29 (1.05)KVN232012 Apr 26
1303 29 1.4+31 14 18.6158.3591-20.5835NGC 1333 IRAS2A East44 GHz (I)
10.03 (0.17)4.66 (0.27)1.216.02 (0.42)KVN622012 Mar 20
1403 29 1.4+31 14 18.6158.3591-20.5835NGC 1333 IRAS2A East44 GHz (I)
10.03 (0.27)4.77 (0.62)0.814.11 (0.15)KVN622012 Mar 20
1503 29 1.4+31 14 18.6158.3591-20.5835NGC 1333 IRAS2A East95 GHz (I)
9.25 (0.44)3.85 (0.78)3.3613.75 (3.34)KVN322012 Mar 20
1603 29 1.4+31 14 18.6158.3591-20.5835NGC 1333 IRAS2A East95 GHz (I)
12.83 (0.96)2.94 (1.20)1.294.03 (2.97)KVN322012 Mar 20
1703 29 1.4+31 14 18.6158.3591-20.5835NGC 1333 IRAS2A East132.8 GHz (I)
8.56 (0.10)2.87 (0.22)9.1427.94 (5.74)KVN232012 Mar 20
1803 29 1.4+31 14 18.6158.3591-20.5835NGC 1333 IRAS2A East132.8 GHz (I)
11.24 (0.29)5.14 (0.36)9.5452.16 (6.29)KVN232012 Mar 20
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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 LYO14

    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 LYO14 in (l,b) histograms



    X
    Position of H2O maser detection
    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