We have performed integral field spectroscopy of the planetary nebulae Hen 3-1333 (PNG332.9-09.9) and Hen 2-113 (PNG321.0+03.9), which are unusual in exhibiting dualdust chemistry and multipolar lobes but also ionized by late-type [WC 10] central stars. The spatially resolved velocity distributions of the Hα emission line were used to determine their primary orientations. The integrated Hα emission profiles indicate that Hen 3-1333 and Hen 2-113 expand with velocities of ~32 and 23 km s-1, respectively. The Hubble Space Telescope observations suggest that these planetary nebulae have two pairs of tenuous lobes extending upwardly from their bright compact cores. From three-dimensional geometric models, the primary lobes of Hen 3-1333 and Hen 2-113 were found to have inclination angles of about -30° and 40° relative to the line of sight, and position angles of -15° and 65° measured east of north in the equatorial coordinate system, respectively.
|Number of pages||4|
|Journal||Monthly Notices of the Royal Astronomical Society: Letters|
|Publication status||Published - 1 May 2015|
Bibliographical noteCopyright 2015 The Authors. First published in Monthly Notices of the Royal Astronomical Society, 449(1), L56-L59. The original publication is available at http://doi.org/10.1093/mnrasl/slv022, published by Oxford University Press on behalf of the Royal Astronomical Society. Version archived for private and non-commercial use with the permission of the author/s and according to publisher conditions. For further rights please contact the publisher.
- ISM: kinematics and dynamics
- Planetary nebulae: general