Journal
ASTROPHYSICAL JOURNAL
Volume 722, Issue 1, Pages 273-280Publisher
IOP PUBLISHING LTD
DOI: 10.1088/0004-637X/722/1/273
Keywords
ISM: molecules; planetary nebulae: individual (NGC 7027)
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Funding
- NSC [96-2112-M-001-018-MY3]
- Research Grants Council of the Hong Kong Special Administrative Region, China [HKU 7031/10P]
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Highly collimated multiple bipolar flows are detected with a 3 '' resolution in the HCO(+) (J = 3-2) and HCN (J = 3-2) lines in the young planetary nebula NGC 7027 with the Submillimeter Array. The HCO(+) and HCN flows coincide in location and velocity with compact and fast CO flows detected with similar to 6 '' resolutions with other millimeter arrays. The equatorial molecular torus of NGC 7027 is captured in HCO(+) emission in the present observations. The HCO(+) emission also closely follows the H(2) emission, indicating that the present observations probe the photon-dominated region of the molecular envelope of NGC 7027.
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