Published September 1, 2022
| Version v1
Poster
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Multi-transitional SHAPEMOL modelling of M1-92: the discovery of a shock excited hot molecular component
Authors/Creators
- 1. UCM (Spain), OAN (Spain)
- 2. OAN (Spain)
- 3. ICMM (Spain)
- 4. IRAM (France)
- 5. CAB (Spain)
Description
M1-92, a.k.a. Minkoski's Footprint nebula, is a pre-planetary nebula (pPN) well studied at a wide range of wavelengths (from cm-radio waves to the optical).
We have used NOEMA maps and single-dish data from CO isotopologues to model M1-92 with SHAPE and SHAPEMOL in order to obtain more information about the nebula and its evolution.
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Poster_SEA2022.pdf
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Additional details
References
- Alcolea, J., Agúndez, M., Bujarrabal, V., et al. (2022). M1-92 Revisited: New Findings and Open Questions: New NOEMA Observations of Minkowski's Footprint. Galaxies, 10(2): 47. doi:10.3390/galaxies10020047.
- Böhm, K.-H. & Solf, J. (1994). A Sub-Arcsecond--Scale Spectroscopic Study of the Complex Mass Outflows in the Vicinity of T Tauri. Astrophysical Journal, 430: 277. doi:10.1086/174402
- Bujarrabal, V., Alcolea, J., Neri, R., et al. (1997). The mass and temperature distribution in the protoplanetary nebula M1-92: 13CO interferometric observations. Astronomy and Astrophysics, 320: 540-522.
- Santander-García, M., Bujarrabal, V., Koning, N., et al. (2015). SHAPEMOL: a 3D code for calculating CO line emission in planetary and protoplanetary nebulae. Astronomy and Astrophysics, 573: A56. doi:10.1051/0004-6361/201322348
- Steffen, W., Koning, N., Wenger, S., et al. (2007). Shape: A 3D Modeling Tool for Astrophysics. IEEE Transactions on Visualization and Computer Graphics, 6:1. doi:10.48550/arXiv.1003.2012