Archivio istituzionale della ricerca dell'Università degli Studi di Palermo
IRIS è il sistema di gestione integrata dei dati della ricerca (persone, pubblicazioni, progetti, attività) adottato dall’Università di Palermo, e ha lo scopo di raccogliere, conservare, documentare, e diffondere ad accesso aperto le informazioni relative alla produzione scientifica degli autori afferenti all’Ateneo.
EnglishAccretion of matter is a process that plays a central role in the physics of young stellar objects. The analysis of the structure by which matter settles on the star can unveil key information about the process of star formation by providing details on mass accretion rates, stellar magnetic field configurations, possible effects of accretion on the stellar coronal activity, etc. Here we review some of the achievements obtained by our group by exploiting a multi-disciplinary approach based on the analysis of multi-dimensional magnetohydrodynamic simulations, multi-wavelength observations, and laboratory experiments of accretion impacts occurring onto the surface of classical T Tauri stars (CTTSs).
Orlando S., Argiroffi C., Bonito R., Colombo S., Peres G., Reale F., et al. (2019). Mass Accretion Impacts in Classical T Tauri Stars: A Multi-disciplinary Approach. In Astrophysics and Space Science Proceedings (pp. 43-48). Springer Netherlands [10.1007/978-3-030-14128-8_6].
| Data di pubblicazione: | 2019 | |
| Titolo: | Mass Accretion Impacts in Classical T Tauri Stars: A Multi-disciplinary Approach | |
| Autori: | ||
| Citazione: | Orlando S., Argiroffi C., Bonito R., Colombo S., Peres G., Reale F., et al. (2019). Mass Accretion Impacts in Classical T Tauri Stars: A Multi-disciplinary Approach. In Astrophysics and Space Science Proceedings (pp. 43-48). Springer Netherlands [10.1007/978-3-030-14128-8_6]. | |
| Abstract: | Accretion of matter is a process that plays a central role in the physics of young stellar objects. The analysis of the structure by which matter settles on the star can unveil key information about the process of star formation by providing details on mass accretion rates, stellar magnetic field configurations, possible effects of accretion on the stellar coronal activity, etc. Here we review some of the achievements obtained by our group by exploiting a multi-disciplinary approach based on the analysis of multi-dimensional magnetohydrodynamic simulations, multi-wavelength observations, and laboratory experiments of accretion impacts occurring onto the surface of classical T Tauri stars (CTTSs). | |
| URL: | http://www.springer.com/series/7395 | |
| ISBN: | 9783030141271 | |
| Digital Object Identifier (DOI): | 10.1007/978-3-030-14128-8_6 | |
| Settore Scientifico Disciplinare: | Settore FIS/05 - Astronomia E Astrofisica | |
| Appare nelle tipologie: | 2.07 Contributo in atti di convegno pubblicato in volume |
File in questo prodotto:
| File | Descrizione | Tipologia | Licenza | |
|---|---|---|---|---|
| Orlando2019_Chapter_MassAccretionImpactsInClassica.pdf | articolo principale | Versione Editoriale | Open Access Visualizza/Apri |
Copyright © 2022