Why Magnetic Fields Cannot Be the Main Agent Shaping Planetary Nebulae-Reference-Cited by-同舟云学术

Why Magnetic Fields Cannot Be the Main Agent Shaping Planetary Nebulae

Published:2006-02 Issue:840 Volume:118 Page:260-269
ISSN:0004-6280
Container-title:Publications of the Astronomical Society of the Pacific
language:en
Short-container-title:PUBL ASTRON SOC PAC

Author:

Soker Noam

Publisher

IOP Publishing

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference44 articles.

1. Bains, I., Gledhill, T. M., Richards, A. M. S. & Yates, J. A. 2004a, in ASP Conf. Ser. 313, Asymmetrical Planetary Nebulae III, ed. M. Meixner et al. (San Francisco: ASP), 186

2. MERLIN polarimetry of the OH masers in OH17.7-2.0

3. MERLIN polarimetry of the OH masers in IRAS 20406+2953

4. Shapes and Shaping of Planetary Nebulae

5. Dynamos in asymptotic-giant-branch stars as the origin of magnetic fields shaping planetary nebulae

Cited by 70 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. The evolutionary route to form planetary nebulae with central neutron star–white dwarf binary systems;Monthly Notices of the Royal Astronomical Society;2023-10-13

2. Morpho-kinematic Properties of Wolf–Rayet Planetary Nebulae;The Astrophysical Journal Supplement Series;2022-05-01

3. Morphologies of Wolf–Rayet Planetary Nebulae Based on IFU Observations;Galaxies;2022-03-08

4. (Sub)stellar companions shape the winds of evolved stars;Science;2020-09-18

5. Mapping Circumstellar Magnetic Fields of Late-type Evolved Stars with the Goldreich–Kylafis Effect: CARMA Observations at λ1.3 mm of R Crt and R Leo;The Astrophysical Journal;2020-08-25