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PIH11 - Expanded Very Large Array Detection of 44.1 GHz Class I Methanol Masers in Sagittarius A

  Interferometry data

Short title: Pihlstrom et al. (2011)
Authors: Pihlstrom, Y. M. Sjouwerman, L. O. Fish, V. L.
Journal: The Astrophysical Journal Letters, Volume 739, Issue 1, article id. L21, 6 pp. (2011).
Bibcode: 2011ApJ...739L..21P

Detection table from Pihlstrom et al. (2011)

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ID Obs. RA Obs. Dec RA offset Dec offset l b Group id # Location Source name Image Line Vpeak Fpeak ∫F dv Telescope Beam Detection Date
(J2000) (J2000) (arcsec) (arcsec) (deg.) (deg.) CH3OH (class I) (km/s) (Jy/beam) (Jy/beam*km/s) (arcsec) Yes/No
1+17 45 38.92-29 00 21359.943809-0.041648G359.985-0.050
Sgr A Image 44 GHz (I)
0.13 .. 2.42 .. NRAOVLA1.3 x 0.5+H2O +CH3OH I +CH3OH II +OH +SiO 2010 October 16
+17 45 38.92-29 00 210 mas0 mas359.943809-0.0416481CalibratorSgr A440.13
+17 45 43.94-29 00 19.575.29881.4988359.953693-0.0570472CSgr ACalibrator2.1
+17 45 49.36-28 58 53.3156.59987.6988359.984421-0.0614413ESgr A45.20.93
+17 45 49.56-28 59 0.6159.59980.3988359.983070-0.0631194ESgr A46.51.43
+17 45 49.67-28 58 55.2161.24985.7988359.984559-0.0626815ESgr A42.72.42
+17 45 49.89-28 59 4.5164.54976.4988359.982771-0.0647106ESgr A36.91.47
+17 45 50.48-29 00 05173.39915.9988359.969542-0.0752967DSgr A49.90.55
+17 45 50.48-28 58 48.7173.39992.2988359.987638-0.0642618ESgr A59.50.5
+17 45 50.49-28 59 7.6173.54973.3988359.983174-0.0670269ESgr A42.80.45
+17 45 50.65-28 59 8.8175.94972.1988359.983193-0.06769710ESgr A280.74
+17 45 51.41-28 59 10.2187.34970.7988359.984303-0.07026411ESgr A44.20.45
+17 45 51.55-28 58 53.7189.44987.2988359.988482-0.06831412ESgr A46.70.51
+17 45 51.62-28 58 26.5190.499114.499359.995066-0.06459913ESgr A52.70.56
+17 45 51.88-28 58 52.9194.39988.0988359.989298-0.06922514ESgr A47.12.39
+17 45 52.12-28 58 55.4197.99985.5988359.989161-0.07033415ESgr A45.90.64
+17 45 52.16-28 58 22.3198.599118.699359.997087-0.06567216ESgr A55.41.11
+17 45 52.43-28 58 58.2202.64982.7988359.989085-0.07170317ESgr A43.70.58
+17 45 52.55-28 58 56.8204.44984.1988359.989644-0.07187418ESgr A45.70.6
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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

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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 PIH11

    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 PIH11 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