Display data from paper

Data: H2O, CH3OH_I

CHO12 - Water and Methanol Maser Activities in the NGC 2024 FIR 6 Region

Short title: Choi et al. (2012)
Authors: Choi, Minho Kang, Miju Byun, Do-Young Lee, Jeong-Eun
Journal: The Astrophysical Journal, Volume 759, Issue 2, article id. 136, 7 pp. (2012).
Bibcode: 2012ApJ...759..136C

PDF: CHO12.pdf

Detection table from Choi et al. (2012)

Export table to csv

Hide / Show individual components

ID Obs. RA Obs. Dec l b Source name 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)
105 41 45.1-01 56 4.4206.5654-16.3618NGC 2024 FIR 644 GHz (I)
11.12 (0.08)2.2 (0.2)1.43.2 (0.2)KVN622011-2012
205 41 45.1-01 56 4.4206.5654-16.3618NGC 2024 FIR 695 GHz (I)
10.99 (0.13)1.8 (0.3)2.54.7 (0.7)KVN292011-2012
305 41 45.1-01 56 4.4206.5654-16.3618NGC 2024 FIR 6132.8 GHz (I)
10.41 (0.19)1.7 (0.4)7.713.7 (2.7)KVN222011-2012
×

Non-detection table from Choi et al. (2012)

Export table to csv

Hide / Show individual components

ID Obs. RA Obs. Dec l b Source name Line Telescope RMS Date
(J2000) (J2000) (deg.) (deg.) CH3OH (class I) (Jy)
105 41 45.1-01 56 4.4206.5654-16.3618NGC 2024 FIR 612(2)->11(1)_A- vt = 1
KVN0.1602011-2012
205 41 45.1-01 56 4.4206.5654-16.3618NGC 2024 FIR 623 GHz (II)
KVN0.1402011-2012
305 41 45.1-01 56 4.4206.5654-16.3618NGC 2024 FIR 66(2)->7(1)_E
KVN0.2702011-2012
405 41 45.1-01 56 4.4206.5654-16.3618NGC 2024 FIR 686.6 GHz (II)
KVN0.2402011-2012
505 41 45.1-01 56 4.4206.5654-16.3618NGC 2024 FIR 686.9 GHz (II)
KVN0.2102011-2012
605 41 45.1-01 56 4.4206.5654-16.3618NGC 2024 FIR 615(3)->14(4)_A+
KVN0.2302011-2012
705 41 45.1-01 56 4.4206.5654-16.3618NGC 2024 FIR 615(3)->14(4)_A-
KVN0.2102011-2012
805 41 45.1-01 56 4.4206.5654-16.3618NGC 2024 FIR 68(4)->9(3)_E
KVN0.3102011-2012
905 41 45.1-01 56 4.4206.5654-16.3618NGC 2024 FIR 620(3)->19(2)_E vt = 1
KVN0.2902011-2012
1005 41 45.1-01 56 4.4206.5654-16.3618NGC 2024 FIR 694 GHz (II)
KVN0.3102011-2012
1105 41 45.1-01 56 4.4206.5654-16.3618NGC 2024 FIR 66(0)->5(1)_E
KVN0.4502011-2012
1205 41 45.1-01 56 4.4206.5654-16.3618NGC 2024 FIR 612(1)->11(2)_A-
KVN0.4102011-2012
1305 41 45.1-01 56 4.4206.5654-16.3618NGC 2024 FIR 6132.6 GHz (II)
KVN0.4302011-2012
1405 41 45.1-01 56 4.4206.5654-16.3618NGC 2024 FIR 65(2)->6(1)_E
KVN0.8702011-2012
1505 41 45.1-01 56 4.4206.5654-16.3618NGC 2024 FIR 612(3)->13(2)_E
KVN0.3702011-2012
1605 41 45.1-01 56 4.4206.5654-16.3618NGC 2024 FIR 67(4)->8(3)_E
KVN0.4102011-2012
1705 41 45.1-01 56 4.4206.5654-16.3618NGC 2024 FIR 623(2)->23(1)_E
KVN0.5702011-2012
1805 41 45.1-01 56 4.4206.5654-16.3618NGC 2024 FIR 618(0)->18(1)_E
KVN0.3802011-2012
1905 41 45.1-01 56 4.4206.5654-16.3618NGC 2024 FIR 60(0)->1(1)_E vt = 1
KVN0.5202011-2012
×
  • Distribution of sources in all sky (l,b)

    Save as PNG, Save as EPS

  • 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 CHO12

    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 CHO12 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