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  • Cambridge University Press (CUP)  (2)
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  • Cambridge University Press (CUP)  (2)
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  • 1
    Online Resource
    Online Resource
    Cambridge University Press (CUP) ; 1997
    In:  Symposium - International Astronomical Union Vol. 170 ( 1997), p. 33-35
    In: Symposium - International Astronomical Union, Cambridge University Press (CUP), Vol. 170 ( 1997), p. 33-35
    Abstract: The Ursa Major molecular cloud complex lies in the direction of an expanding HI shell known as the North Celestial Pole loop. The NCP loop, which is centered at ( l , b ) ∼ (138°,30°) and easily seen in IRAS 100 μm emission, is some 60 pc across and 150 pc distant (Meyerdierks et. al 1991). At 100 μm, the Ursa Major clouds appear in projection as “finger” ( l ∼ 140, b ∼ 38) which “hangs down” towards the center of the loop and the plane of the Galaxy. Distance estimates to the molecular clouds (Penprase 1993) are consistent with that of the NCP loop, indicating that the clouds are physically associated with the loop.
    Type of Medium: Online Resource
    ISSN: 0074-1809
    Language: English
    Publisher: Cambridge University Press (CUP)
    Publication Date: 1997
    SSG: 16,12
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  • 2
    Online Resource
    Online Resource
    Cambridge University Press (CUP) ; 2013
    In:  Proceedings of the International Astronomical Union Vol. 9, No. S303 ( 2013-10), p. 114-116
    In: Proceedings of the International Astronomical Union, Cambridge University Press (CUP), Vol. 9, No. S303 ( 2013-10), p. 114-116
    Abstract: Because of its large angular extent, the central molecular zone (CMZ) has to date only been mapped in the mm with single dish telescopes, with resolution about 30″ (1.4 pc). We present the first interferometric maps of a 90 × 50 pc region of the CMZ, with spatial resolution of ∼10″ (0.4 pc). We mapped ∼0.25 square degrees of the CMZ with CARMA in 3mm continuum and the spectral lines SiO J = (2 − 1), HCO + J = (1 − 0), HCN J = (1 − 0), N 2 H + J = (1 − 0), and CS J = (2 − 1), covering roughly V LSR = −200 to 200 km s −1 with spectral resolution ΔV ∼ 2.5 km s −1 . To recover the large scale structure resolved out by the interferometer, the continuum-subtracted spectral line images were combined with the Mopra 22-m telescope survey.
    Type of Medium: Online Resource
    ISSN: 1743-9213 , 1743-9221
    Language: English
    Publisher: Cambridge University Press (CUP)
    Publication Date: 2013
    detail.hit.zdb_id: 2170724-8
    SSG: 16,12
    Location Call Number Limitation Availability
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