Zobrazeno 1 - 10
of 29
pro vyhledávání: '"de Wit, Stephan"'
Autor:
Maravelias, Grigoris, de Wit, Stephan, Bonanos, Alceste Z., Tramper, Frank, Munoz-Sanchez, Gonzalo, Christodoulou, Evangelia
Publikováno v:
Galaxies 2023, 11(3), 79
Mass loss is one of the key parameters that determine stellar evolution. Despite the progress we have achieved over the last decades we still cannot match the observational derived values with theoretical predictions. Even worse, there are certain ph
Externí odkaz:
http://arxiv.org/abs/2307.03320
Autor:
Yang, Ming, Bonanos, Alceste Z., Jiang, Biwei, Zapartas, Emmanouil, Gao, Jian, Ren, Yi, Lam, Man I, Wang, Tianding, Maravelias, Grigoris, Gavras, Panagiotis, Wang, Shu, Chen, Xiaodian, Tramper, Frank, de Wit, Stephan, Chen, Bingqiu, Wen, Jing, Liu, Jiaming, Tian, Hao, Antoniadis, Konstantinos, Luo, Changqing
Publikováno v:
A&A 676, A84 (2023)
We assemble the most complete and clean red supergiant (RSG) sample (2,121 targets) so far in the Small Magellanic Cloud (SMC) with 53 different bands of data to study the MLR of RSGs. In order to match the observed spectral energy distributions (SED
Externí odkaz:
http://arxiv.org/abs/2304.01835
Autor:
Maravelias, Grigoris, Bonanos, Alceste Z., Tramper, Frank, de Wit, Stephan, Yang, Ming, Bonfini, Paolo, Zapartas, Emmanuel, Antoniadis, Konstantinos, Christodoulou, Evangelia, Muñoz-Sanchez, Gonzalo
Mass loss is a key property to understand stellar evolution and in particular for low-metallicity environments. Our knowledge has improved dramatically over the last decades both for single and binary evolutionary models. However, episodic mass loss
Externí odkaz:
http://arxiv.org/abs/2209.06303
Autor:
Maravelias, Grigoris, Bonanos, Alceste Z., Tramper, Frank, de Wit, Stephan, Yang, Ming, Bonfini, Paolo
Publikováno v:
A&A 666, A122 (2022)
(abridged) Mass loss is a key parameter in the evolution of massive stars, with discrepancies between theory and observations and with unknown importance of the episodic mass loss. To address this we need increased numbers of classified sources stars
Externí odkaz:
http://arxiv.org/abs/2203.08125
Autor:
Lobo, Suzana Margareth, Plantefève, Gaétan, Nair, Girish, Joaquim Cavalcante, Adilson, Franzin de Moraes, Nara, Nunes, Estevao, Barnum, Otis, Berdun Stadnik, Claudio Marcel, Lima, Maria Patelli, Lins, Muriel, Hajjar, Ludhmila Abrahao, Lipinski, Christopher, Islam, Shaheen, Ramos, Fabiano, Simon, Tiago, Martinot, Jean-Benoît, Guimard, Thomas, Desclaux, Arnaud, Lioger, Bertrand, Neuenschwander, Fernando Carvalho, DeSouza Paolino, Bruno, Amin, Alpesh, Acosta, Samuel Amil, Dilling, Daniel Forde, Cartagena, Edgardo, Snyder, Brian, Devaud, Edouard, Barreto Berselli Marinho, Ana Karolina, Tanni, Suzana, Milhomem Beato, Patricia Medeiros, De Wit, Stephan, Selvan, Vani, Gray, Jeffrey, Fernandez, Ricardo, Pourcher, Valérie, Maddox, Lee, Kay, Richard, Azbekyan, Anait, Chabane, Mounia, Tourette, Cendrine, Esmeraldino, Luis Everton, Dilda, Pierre J., Lafont, René, Mariani, Jean, Camelo, Serge, Rabut, Sandrine, Agus, Samuel, Veillet, Stanislas, Dioh, Waly, van Maanen, Rob, Morelot-Panzini, Capucine
Publikováno v:
In eClinicalMedicine February 2024 68
Autor:
Maravelias, Grigoris, Bonanos, Alceste Z., Tramper, Frank, de Wit, Stephan, Yang, Ming, Bonfini, Paolo, Zapartas, Emmanuel, Antoniadis, Konstantinos, Christodoulou, Evangelia, Muñoz-Sanchez, Gonzalo
Publikováno v:
Proceedings of the International Astronomical Union; May2024, Vol. 18 Issue S361, p454-459, 6p
Autor:
Maravelias, Grigoris, Bonanos, Alceste Z., Tramper, Frank, de Wit, Stephan, Yang, Ming, Bonfini, Paolo, Zapartas, Manos, Antoniadis, Konstantinos, Christodoulou, Evangelia, Munoz-Sanchez, Gonzalo
Although our knowledge on stellar evolution has improved dramatically over the last decades, both regarding single and binary evolutionary models, we still lack pieces of the puzzle. Mass loss is a key property to understand and characterize stellar
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2916b74db45865bfdcb1177655346869
Autor:
Maravelias, Grigoris, de Wit, Stephan, Bonanos, Alceste Z., Tramper, Frank, Munoz-Sanchez, Gonzalo, Christodoulou, Evangelia
Mass loss is one of the key parameters that determine stellar evolution. Despite the progress we have achieved over the last decades we still cannot match the observational derived values with theoretical predictions. Even worse, there are certain ph
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0a0da0dc1a09b11a6212cde36de3ff9e
Autor:
Christodoulou, Evangelia, Bonanos, Alceste, Sanchez, Gonzalo Munoz, De Wit, Stephan, Grigoris Maravelias, Alvarez, David Garcia, Antoniadis, Kostas
The role of episodic mass loss in the evolution of massive stars remains largely unknown and thus it is not included in the stellar models. The ASSESS project is conducting an optical survey in the nearby Universe (12 galaxies with Z ~ 0.1 to 1.5 Zo)
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::289d657c04b396b187392e4d1efe2a76
Autor:
Bonanos, Alceste Z., Maravelias, Grigoris, Yang, Ming, Tramper, Frank, de Wit, Stephan, Zapartas, Emmanouil, Antoniadis, Konstantinos, Christodoulou, Evangelia, Munoz-Sanchez, Gonzalo
Episodic mass loss is not understood theoretically, neither accounted for in state-of-the-art models of stellar evolution, which has far-reaching consequences for many areas of astronomy. We present the status and results of the ERC-funded ASSESS pro
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::24504fa85a1f227ae379a3774aef6bce