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NAK15 - Methanol observation of IRAS 19312+1950: A possible new type of class I methanol maser

Short title: Nakashima et al. (2015)
Authors: Nakashima, Jun-ichi Sobolev, Andrej M. Salii, Svetlana V. Zhang, Yong Yung, Bosco H. K. Deguchi, Shuji
Journal: Publications of the Astronomical Society of Japan, Volume 67, Issue 5, id.9512 pp.
Bibcode: 2015PASJ...67...95N

Detection table from Nakashima et al. (2015)

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ID Obs. RA Obs. Dec l b Group id Source name Line Thermal Vpeak ∫Ta dv Telescope RMS Beam Detection Date
(J2000) (J2000) (deg.) (deg.) CH3OH (class I) line mark (km/s) (K*km/s) (Jy) (arcsec) Yes/No
119 33 24.2+19 56 55.755.37070.1855G55.371+0.185
IRAS 19312+195044 GHz (I)
36.10.56NRO0.03738+H2O +CH3OH I -CH3OH II +OH +SiO 2011 February 11
219 33 24.2+19 56 55.755.37070.1855G55.371+0.185
IRAS 19312+19501(0)->0(0)_A+
*35.80.249NRO0.01834+H2O +CH3OH I -CH3OH II +OH +SiO 2012 March 14-17 and May 14-16
319 33 24.2+19 56 55.755.37070.1855G55.371+0.185
IRAS 19312+195095 GHz (I)
360.115NRO0.00717.6+H2O +CH3OH I -CH3OH II +OH +SiO 2012 March 14-17 and May 14-16
419 33 24.2+19 56 55.755.37070.1855G55.371+0.185
IRAS 19312+19502(-1)->1(-1)_E
*35.80.205NRO0.00917.6+H2O +CH3OH I -CH3OH II +OH +SiO 2012 March 14-17 and May 14-16
519 33 24.2+19 56 55.755.37070.1855G55.371+0.185
IRAS 19312+19502(0)->1(0)_A+
*35.50.228NRO0.00917.6+H2O +CH3OH I -CH3OH II +OH +SiO 2012 March 14-17 and May 14-16
619 33 24.2+19 56 55.755.37070.1855G55.371+0.185
IRAS 19312+19502(0)->1(0)_E
*39.10.064NRO0.00917.6+H2O +CH3OH I -CH3OH II +OH +SiO 2012 March 14-17 and May 14-16
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Non-detection table from Nakashima et al. (2015)

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ID Obs. RA Obs. Dec l b Group id Source name Line Telescope RMS Beam Detection Date
(J2000) (J2000) (deg.) (deg.) CH3OH (class I) (Jy) (arcsec) Yes/No
119 33 24.2+19 56 55.755.37070.1855G55.371+0.185
IRAS 19312+19509(2)->10(1)_A++
NRO0.01072+H2O +CH3OH I -CH3OH II +OH +SiO 2012 March 14-17 and May 14-16
219 33 24.2+19 56 55.755.37070.1855G55.371+0.185
IRAS 19312+195023 GHz (I)
NRO0.01072+H2O +CH3OH I -CH3OH II +OH +SiO 2012 March 14-17 and May 14-16
319 33 24.2+19 56 55.755.37070.1855G55.371+0.185
IRAS 19312+195036 GHz (I)
NRO0.01346+H2O +CH3OH I -CH3OH II +OH +SiO 2012 March 14-17 and May 14-16
419 33 24.2+19 56 55.755.37070.1855G55.371+0.185
IRAS 19312+195044 GHz (I)
NRO0.01338+H2O +CH3OH I -CH3OH II +OH +SiO 2012 March 14-17 and May 14-16
519 33 24.2+19 56 55.755.37070.1855G55.371+0.185
IRAS 19312+19501(0)->0(0)_E
NRO0.02234+H2O +CH3OH I -CH3OH II +OH +SiO 2012 March 14-17 and May 14-16
19 33 24.2+19 56 55.755.37070.1855G55.371+0.185
IRAS 19312+19501(0)->0(0)_E
NRO0.01534+H2O +CH3OH I -CH3OH II +OH +SiO 2012 March 14-17 and May 14-16
619 33 24.2+19 56 55.755.37070.1855G55.371+0.185
IRAS 19312+19508(3,5)->9(2,7)_E
NRO0.00617.8+H2O +CH3OH I -CH3OH II +OH +SiO 2012 March 14-17 and May 14-16
719 33 24.2+19 56 55.755.37070.1855G55.371+0.185
IRAS 19312+195095 GHz (I)
NRO0.00617.6+H2O +CH3OH I -CH3OH II +OH +SiO 2012 March 14-17 and May 14-16
819 33 24.2+19 56 55.755.37070.1855G55.371+0.185
IRAS 19312+19502(1)->1(1) E
NRO0.00417.6+H2O +CH3OH I -CH3OH II +OH +SiO 2012 March 14-17 and May 14-16
919 33 24.2+19 56 55.755.37070.1855G55.371+0.185
IRAS 19312+1950108 GHz (II)
NRO0.01015.5+H2O +CH3OH I -CH3OH II +OH +SiO 2012 March 14-17 and May 14-16
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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 NAK15

    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 NAK15 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