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On the circumstellar envelopes of semi-regular long-period variables

Published online by Cambridge University Press:  30 December 2019

J. J. Díaz-Luis ,
J. Alcolea ,
V. Bujarrabal Open the ORCID record for V. Bujarrabal [Opens in a new window] ,
M. Santander-García ,
M. Gómez-Garrido  and
J.-F. Desmurs
J. J. Díaz-Luis
Affiliation:
Observatorio Astronómico Nacional (IGN), Spain email: jjairo@oan.es
J. Alcolea
Affiliation:
Observatorio Astronómico Nacional (IGN), Spain email: jjairo@oan.es
V. Bujarrabal
Affiliation:
Observatorio Astronómico Nacional (IGN), Spain email: jjairo@oan.es
M. Santander-García
Affiliation:
Observatorio Astronómico Nacional (IGN), Spain email: jjairo@oan.es
M. Gómez-Garrido
Affiliation:
Instituto Geográfico Nacional (IGN), Centro de Desarrollos Tecnológicos, Observatorio de Yebes, Spain
J.-F. Desmurs
Affiliation:
Observatorio Astronómico Nacional (IGN), Spain email: jjairo@oan.es
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Abstract

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The mass loss process along the AGB phase is crucial for the formation of circumstellar envelopes (CSEs), which in the post-AGB phase will evolve into planetary nebulae (PNe). There are still important issues that need to be further explored in this field; in particular, the formation of axially symmetric PNe from spherical CSEs. To address the problem, we have conducted high S/N IRAM 30 m observations of 12COJ = 1−0 and J = 2−1, and 13COJ = 1−0 in a volume-limited unbiased sample of semi-regular variables (SRs). We also conducted Yebes 40 m SiO J = 1−0 observations in 1/2 of the sample in order to complement our 12CO observations. We report a moderate correlation between mass loss rate and the 12CO(1−0)−to−12CO(2−1) line intensity ratio, introducing a possible new method for determining mass loss rates of SRs with short analysis time. We also find that for several stars the SiO profiles are very similar to the 12CO profiles, a totally unexpected result unless these are non-standard envelopes.

Keywords

planetary nebulae: generalstars: AGB and post-AGBmillimeter
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S343: Why Galaxies Care About AGB Stars: A Continuing Challenge through Cosmic Time , August 2018 , pp. 186 - 190
Copyright
© International Astronomical Union 2019 

References

Balick, B., & Frank, A. 2002, ARA&A, 40, 439 CrossRefGoogle Scholar
Castro-Carrizo, A., Quintana-Lacaci, G., Neri, R., et al. 2010, A&A, 523, A59 Google Scholar
Douchin, D., De Marco, O., Frew, D. J., et al. 2015, MNRAS, 448, 3132 CrossRefGoogle Scholar
Groenewegen, M. A. T. 2017, A&A, 606, A67 Google Scholar
Hirano, N., Shinnaga, H., Dinh-V-Trung, et al. 2004, ApJ, 616, L43 CrossRefGoogle Scholar
Homan, W., Richards, A., Decin, L., Kervella, P., de Koter, A., McDonald, I., Ohnaka, K. 2017, A&A, 601, A5 Google Scholar
Homan, W., Richards, A., Decin, L., de Koter, A., Kervella, P. 2018, A&A, 616, A34 Google Scholar
IRAS, 1988, The Point Source Catalogue, version 2.0, NASA RP-1190Google Scholar
Jones, D., & Boffin, H. M. J. 2017, NatAs, 1, 0117 Google Scholar
Kim, H., Liu, S.-Y., Hirano, N., et al. 2015, ApJ, 814, 61 CrossRefGoogle Scholar
Knapp, G. R., & Morris, M. 1985, ApJ, 292, 640 CrossRefGoogle Scholar
Loup, C., Forveille, T., Omont, A., Paul, J. F. 1993, A&AS, 99, 291 Google Scholar
Maercker, M., Mohamed, S., Vlemmings, W. H. T., et al. 2012, Nature, 490, 232 CrossRefGoogle Scholar
Mauron, N., & Huggins, P. J. 2006, A&A, 452, 257 Google Scholar
Morris, M., Sahai, R., Matthews, K., et a l. 2006, in Planetary Nebulae in our Galaxy and Beyond, ed. Barlow, M. J., &Mèndez, R. H., IAU Symp., 234, 469 Google Scholar
Neri, R., Kahane, C., Lucas, R., et al. 1998, A&AS, 130, 1 Google Scholar
Olofsson, H. 1999, in IAU Symposium 191, 3 Google Scholar
Ortiz, R., & Guerrero, M. A. 2016, MNRAS, 461, 3036 CrossRefGoogle Scholar
Parker, Q. A., Acker, A., Frew, D. J., et al. 2006, MNRAS, 373, 79 CrossRefGoogle Scholar
Raghavan, D., McAlister, H. A., Henry, T. J., et al. 2010, ApJS, 190, 1 CrossRefGoogle Scholar
Sahai, R., Findeisen, K., de Paz, Gil, A., et al. 2008, ApJ, 689, 1274 CrossRefGoogle Scholar
Samus, N. N., Durlevich, O. V., Kazarovets, E. V., et al. 2012, GCVS, VizieR On-line Data Catalog: B/gcvsGoogle Scholar
Santander-García, M., Bujarrabal, V., Koning, N., Steffen, W. 2015, A&A, 573, A56 Google Scholar
Steffen, W., Koning, N., Wenger, S., Morisset, C., Magnor, M. 2011, IEEE Transactions on Visualization and Computer Graphics, 17, 454 CrossRefGoogle Scholar
van Leeuwen, F. 2007, A&A, 474, 653 Google Scholar