July 16, 2007Open Access

The massive expanding molecular torus in the planetary nebula NGC 6302

Key Points

Key points are not available for this paper at this time.

Abstract

Aims.We measure the mass and kinematics of the massive molecular torus in the the proto-typical butterfly planetary nebula NGC 6302. Determining the mass-loss history of the source is an important step in understanding the origin and formation of the wing-like morphology.

AIに質問

Bookmark

View Full Paper

Cite This Study

Peretto et al. (Mon,) studied this question.

synapsesocial.com/papers/69d7c2863b601d7be3ae2bbd https://doi.org/https://doi.org/10.1051/0004-6361:20066973

Also Consider

Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context:

1An atomic and molecular database for analysis of submillimetre line observations2005 · 1,554 citations
2On the origin of planetary nebulae1978 · 505 citations
3A search for molecular outflows toward the pre-main-sequence objects1988 · 113 citations
4The accretion of brown dwarfs and planets by giant stars -- I. Asymptotic giant branch stars1999 · 163 citations
5Population Diagram Analysis of Molecular Line Emission1999 · 850 citations

AIに質問

Bookmark

View Full Paper