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Article: Spatially resolved kinematic observations of the planetary nebulae Hen 3-1333 and Hen 2-113
Title | Spatially resolved kinematic observations of the planetary nebulae Hen 3-1333 and Hen 2-113 |
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Authors | |
Keywords | ISM: kinematics and dynamics Planetary nebulae: general Stars:Wolf-Rayet |
Issue Date | 1-May-2015 |
Publisher | Oxford University Press |
Citation | Monthly Notices of the Royal Astronomical Society: Letters, 2015, v. 449, n. 1, p. 56-59 How to Cite? |
Abstract | 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 dual-dust chemistry and multipolar lobes but also ionized by late-type [WC 10] central stars. The spatially resolved velocity distributions of the H alpha emission line were used to determine their primary orientations. The integrated H alpha emission profiles indicate that Hen 3-1333 and Hen 2-113 expand with velocities of similar to 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 -30A degrees and 40A degrees relative to the line of sight, and position angles of -15A degrees and 65A degrees measured east of north in the equatorial coordinate system, respectively. |
Persistent Identifier | http://hdl.handle.net/10722/343529 |
ISSN | 2023 SCImago Journal Rankings: 1.521 |
ISI Accession Number ID |
DC Field | Value | Language |
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dc.contributor.author | Danehkar, A | - |
dc.contributor.author | Parker, QA | - |
dc.date.accessioned | 2024-05-14T05:21:14Z | - |
dc.date.available | 2024-05-14T05:21:14Z | - |
dc.date.issued | 2015-05-01 | - |
dc.identifier.citation | Monthly Notices of the Royal Astronomical Society: Letters, 2015, v. 449, n. 1, p. 56-59 | - |
dc.identifier.issn | 1745-3925 | - |
dc.identifier.uri | http://hdl.handle.net/10722/343529 | - |
dc.description.abstract | 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 dual-dust chemistry and multipolar lobes but also ionized by late-type [WC 10] central stars. The spatially resolved velocity distributions of the H alpha emission line were used to determine their primary orientations. The integrated H alpha emission profiles indicate that Hen 3-1333 and Hen 2-113 expand with velocities of similar to 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 -30A degrees and 40A degrees relative to the line of sight, and position angles of -15A degrees and 65A degrees measured east of north in the equatorial coordinate system, respectively. | - |
dc.language | eng | - |
dc.publisher | Oxford University Press | - |
dc.relation.ispartof | Monthly Notices of the Royal Astronomical Society: Letters | - |
dc.rights | This work is licensed under a Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License. | - |
dc.subject | ISM: kinematics and dynamics | - |
dc.subject | Planetary nebulae: general | - |
dc.subject | Stars:Wolf-Rayet | - |
dc.title | Spatially resolved kinematic observations of the planetary nebulae Hen 3-1333 and Hen 2-113 | - |
dc.type | Article | - |
dc.identifier.doi | 10.1093/mnrasl/slv022 | - |
dc.identifier.scopus | eid_2-s2.0-84926431954 | - |
dc.identifier.volume | 449 | - |
dc.identifier.issue | 1 | - |
dc.identifier.spage | 56 | - |
dc.identifier.epage | 59 | - |
dc.identifier.eissn | 1745-3933 | - |
dc.identifier.isi | WOS:000353555000012 | - |
dc.publisher.place | OXFORD | - |
dc.identifier.issnl | 1745-3933 | - |