Abundance Pattern Analysis of Planet-hosting and Debris-disk Stars
Abstract: About 16 % of the main-sequence solar-like stars are surrounded by dusty debris disks (DD). These disks are the detritus of small bodies collisions and their presence is a very strong signpost of planet formation. One of the most interesting characteristics of stars hosting a giant planet...
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2021
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| Acceso en línea: | http://hdl.handle.net/11086/18938 |
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I10-R141-11086-189382025-03-11T12:15:24Z Abundance Pattern Analysis of Planet-hosting and Debris-disk Stars Chavero, Carolina Andrea. Rojas, M. Drake, N. A. Pereira, C. B. Kholtygin, A. F. Cahuasqui, J. A. Discos circunestelares Abundancia metálica Abstract: About 16 % of the main-sequence solar-like stars are surrounded by dusty debris disks (DD). These disks are the detritus of small bodies collisions and their presence is a very strong signpost of planet formation. One of the most interesting characteristics of stars hosting a giant planet is a direct relationship between metallicity and probability of planet formation, which was found to increase with stellar metallicity Gonzalez (1997). Instead, the small planets would form around host stars (HS) with a wide range of metallicities (Buchhave et al. 2012). On the other hand the presence of debris disks is uncorrelated with metallicity (Chavero et al. 2006, Greaves et al. 2006, Maldonado et al. 2012). Fil: Chavero, Carolina Andrea. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina. Fil: Chavero, Carolina Andrea. Conicet; Argentina. http://www.aspbooks.org/a/volumes/article_details/?paper_id=36464 Fil: Chavero, Carolina Andrea. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba; Argentina. Fil: Chavero, Carolina Andrea. Conicet; Argentina. Astronomía (incluye Astrofísica y Ciencias del Espacio) 2021-07-07T21:02:55Z 2021-07-07T21:02:55Z 2014 conferenceObject 978-1-58381-849-7 http://hdl.handle.net/11086/18938 eng Attribution-NonCommercial-ShareAlike 4.0 International https://creativecommons.org/licenses/by-nc-sa/4.0/ Electrónico y/o Digital |
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Universidad Nacional de Córdoba |
| institution_str |
I-10 |
| repository_str |
R-141 |
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Repositorio Digital Universitario (UNC) |
| language |
Inglés |
| topic |
Discos circunestelares Abundancia metálica |
| spellingShingle |
Discos circunestelares Abundancia metálica Chavero, Carolina Andrea. Rojas, M. Drake, N. A. Pereira, C. B. Kholtygin, A. F. Cahuasqui, J. A. Abundance Pattern Analysis of Planet-hosting and Debris-disk Stars |
| topic_facet |
Discos circunestelares Abundancia metálica |
| description |
Abstract: About 16 % of the main-sequence solar-like stars are surrounded by dusty debris disks (DD). These disks are the detritus of small bodies collisions and their presence is a very strong signpost of planet formation. One of the most interesting characteristics of stars hosting a giant planet is a direct relationship between metallicity and probability of planet formation, which was found to increase with stellar metallicity Gonzalez (1997). Instead, the small planets would form around host stars (HS) with a wide range of metallicities (Buchhave et al. 2012). On the other hand the presence of debris disks is uncorrelated with metallicity (Chavero et al. 2006, Greaves et al. 2006, Maldonado et al. 2012). |
| format |
conferenceObject |
| author |
Chavero, Carolina Andrea. Rojas, M. Drake, N. A. Pereira, C. B. Kholtygin, A. F. Cahuasqui, J. A. |
| author_facet |
Chavero, Carolina Andrea. Rojas, M. Drake, N. A. Pereira, C. B. Kholtygin, A. F. Cahuasqui, J. A. |
| author_sort |
Chavero, Carolina Andrea. |
| title |
Abundance Pattern Analysis of Planet-hosting and Debris-disk Stars |
| title_short |
Abundance Pattern Analysis of Planet-hosting and Debris-disk Stars |
| title_full |
Abundance Pattern Analysis of Planet-hosting and Debris-disk Stars |
| title_fullStr |
Abundance Pattern Analysis of Planet-hosting and Debris-disk Stars |
| title_full_unstemmed |
Abundance Pattern Analysis of Planet-hosting and Debris-disk Stars |
| title_sort |
abundance pattern analysis of planet-hosting and debris-disk stars |
| publishDate |
2021 |
| url |
http://hdl.handle.net/11086/18938 |
| work_keys_str_mv |
AT chaverocarolinaandrea abundancepatternanalysisofplanethostinganddebrisdiskstars AT rojasm abundancepatternanalysisofplanethostinganddebrisdiskstars AT drakena abundancepatternanalysisofplanethostinganddebrisdiskstars AT pereiracb abundancepatternanalysisofplanethostinganddebrisdiskstars AT kholtyginaf abundancepatternanalysisofplanethostinganddebrisdiskstars AT cahuasquija abundancepatternanalysisofplanethostinganddebrisdiskstars |
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