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ZUC89 - Carbon stars with oxygen-rich circumstellar envelopes?

Short title: Zuckerman & Maddalena (1989)
Authors: Zuckerman, B. Maddalena, R. J.
Journal: Astronomy and Astrophysics (ISSN 0004-6361), vol. 223, no. 1-2, Oct. 1989, p. L20-L22.
Bibcode: 1989A&A...223L..20Z

Detection table from Zuckerman & Maddalena (1989)

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Non-detection table from Zuckerman & Maddalena (1989)

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ID Obs. RA Obs. Dec l b Group id Source name Line Fpeak List Detection Class Ref.
(J2000) (J2000) (deg.) (deg.) OH (Jy) Yes/No
121 43 16.3+38 01 0386.9106-11.3600G86.911-11.360
RV Cyg1.612 GHz; 0.180ENG15-OH EVOLVEDZUC89
221 42 1.1+35 30 36.785.0053-13.0577G85.005-13.058
V460 Cyg1.667 GHz; 0.300ENG15-H2O -OH EVOLVEDZUC89
321 42 1.1+35 30 36.785.0053-13.0577G85.005-13.058
V460 Cyg1.665 GHz; 0.240ENG15-H2O -OH EVOLVEDZUC89
421 42 1.1+35 30 36.785.0053-13.0577G85.005-13.058
V460 Cyg1.612 GHz; 0.180ENG15-H2O -OH EVOLVEDZUC89
518 50 20-07 54 27.425.7610-3.3529G25.761-3.353
S Sct1.667 GHz; 0.300ENG15-H2O -OH EVOLVEDZUC89
618 50 20-07 54 27.425.7610-3.3529G25.761-3.353
S Sct1.665 GHz; 0.240ENG15-H2O -OH EVOLVEDZUC89
718 50 20-07 54 27.425.7610-3.3529G25.761-3.353
S Sct1.612 GHz; 0.240ENG15-H2O -OH EVOLVEDZUC89
810 51 37.3-21 15 0.3268.964933.6014G268.965+33.601
V Hya1.667 GHz; 0.240ENG15-H2O -OH +SiO EVOLVEDZUC89
910 51 37.3-21 15 0.3268.964933.6014G268.965+33.601
V Hya1.665 GHz; 0.240ENG15-H2O -OH +SiO EVOLVEDZUC89
1010 51 37.3-21 15 0.3268.964933.6014G268.965+33.601
V Hya1.612 GHz; 0.240ENG15-H2O -OH +SiO EVOLVEDZUC89
1110 35 12.9-39 33 45.3276.224116.1419G276.224+16.142
U Ant1.667 GHz; 0.240ENG15-OH EVOLVEDZUC89
1210 35 12.9-39 33 45.3276.224116.1419G276.224+16.142
U Ant1.665 GHz; 0.300ENG15-OH EVOLVEDZUC89
1303 41 48.2+62 38 54.4141.14995.9679G141.150+5.968
U Cam1.665 GHz; 0.090ENG15-OH EVOLVEDZUC89
1403 41 48.2+62 38 54.4141.14995.9679G141.150+5.968
U Cam1.612 GHz; 0.090ENG15-OH EVOLVEDZUC89
1501 26 58.1-32 32 35.4250.1812-80.5886G250.181-80.589
R Scl1.667 GHz; 0.300ENG15-H2O -OH EVOLVEDZUC89
1601 26 58.1-32 32 35.4250.1812-80.5886G250.181-80.589
R Scl1.665 GHz; 0.240ENG15-H2O -OH EVOLVEDZUC89
1710 35 12.9-39 33 45.3276.224116.1419G276.224+16.142
U Ant1.612 GHz; 0.180ENG15-OH EVOLVEDZUC89
1803 41 48.2+62 38 54.4141.14995.9679G141.150+5.968
U Cam1.667 GHz; 0.180ENG15-OH EVOLVEDZUC89
1901 26 58.1-32 32 35.4250.1812-80.5886G250.181-80.589
R Scl1.612 GHz; 0.180ENG15-H2O -OH EVOLVEDZUC89
2021 43 16.3+38 01 0386.9106-11.3600G86.911-11.360
RV Cyg1.665 GHz; 0.240ENG15-OH EVOLVEDZUC89
2121 43 16.3+38 01 0386.9106-11.3600G86.911-11.360
RV Cyg1.667 GHz; 0.240ENG15-OH EVOLVEDZUC89
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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 ZUC89

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    Longitude-Velocity Map is taken form Dame, Hartmann & Thaddeus (2001)

  • Distribution of sources from ZUC89 in (l,b) histograms



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    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

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    2MASS K

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