No CrossRef data available.
Article contents
Evidence of Jets in the Bipolar Planetary Nebulae M 1-91 and M 1-92
Published online by Cambridge University Press: 26 May 2016
Abstract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
For M1-91 we find that the ratio of the 6717/6731 [S II] narrow band images shows two symmetrical very collimated high density regions, or jets, along the major axis.
We infer many properties of M 1-92 from the similarity of the spectral features with the symbiotic star MWC 560. We show that M 1-92 could also have a jet along the major axis and that from the NW knot we receive scattered light from the central region that has traveled along the line of symmetry.
- Type
- Part VII: Nebular Morphology and Dynamics
- Information
- Copyright
- Copyright © Astronomical Society of the Pacific 2003
References
Bujarrabal, V., Alcolea, J., Sahai, R., Zamorano, J. & Zijlstra, A. A.
1998, A&A, 331, 361
Google Scholar
Machado, A., Guerrero, M. A., Stanghellini, L. and Serra-Ricart, M.
1996, The IAC Morphological Catalog of Northern Galactic Planetary Nebulae
CrossRefGoogle Scholar
Schmid, H. M., Kaufer, A., Camenzind, M., Rivinius, Th., Stahl, O., Szeifert, T.
Tubbesing, S., & Wolf, B.
2001, A&A, 377, 206
Google Scholar