Zobrazeno 1 - 10
of 812
pro vyhledávání: '"P. Bonanos"'
Autor:
Munoz-Sanchez, G., Kalitsounaki, M., de Wit, S., Antoniadis, K., Bonanos, A. Z., Zapartas, E., Boutsia, K., Christodoulou, E., Maravelias, G., Soszynski, I., Udalski, A.
Red Supergiants (RSGs) are cool, evolved massive stars in their final evolutionary stage before exploding as a supernova. However, the evolution and fate of the most luminous RSGs is uncertain. Observational evidence for luminous warm, post-RSG objec
Externí odkaz:
http://arxiv.org/abs/2411.19329
Autor:
Zapartas, E., de Wit, S., Antoniadis, K., Muñoz-Sanchez, G., Souropanis, D., Bonanos, A. Z., Maravelias, G., Kovlakas, K., Kruckow, M. U., Fragos, T., Andrews, J. J., Bavera, S. S., Briel, M., Gossage, S., Kasdagli, E., Rocha, K. A., Sun, M., Srivastava, P. M., Xing, Z.
The rate and mechanism of mass loss of red supergiants (RSGs) remain poorly understood, especially at low metallicities. Motivated by the new empirical prescription by Yang et al. 2023, based on the largest and most complete sample in the Small Magel
Externí odkaz:
http://arxiv.org/abs/2410.07335
Autor:
de Wit, S., Bonanos, A. Z., Antoniadis, K., Zapartas, E., Ruiz, A., Britavskiy, N., Christodoulou, E., De, K., Maravelias, G., Munoz-Sanchez, G., Tsopela, A.
Publikováno v:
A&A 689, A46 (2024)
Mass loss during the red supergiant (RSG) phase plays a crucial role in the evolution of an intermediate massive star, however, the underlying mechanism remains unknown. We aim to increase the sample of well-characterized RSGs at subsolar metallicity
Externí odkaz:
http://arxiv.org/abs/2402.12442
Autor:
Munoz-Sanchez, G., de Wit, S., Bonanos, A. Z., Antoniadis, K., Boutsia, K., Boumis, P., Christodoulou, E., Kalitsounaki, M., Udalski, A.
Publikováno v:
A&A 690, A99 (2024)
This study delves into [W60] B90, one of the most luminous and extreme Red Supergiants (RSGs) in the Large Magellanic Cloud (LMC), aiming to search for evidence of episodic mass loss. Our discovery of a bar-like nebular structure at 1 pc, reminiscent
Externí odkaz:
http://arxiv.org/abs/2405.11019
Autor:
Dong, Yize, Tsuna, Daichi, Valenti, Stefano, Sand, David J., Andrews, Jennifer E., Bostroem, K. Azalee, Hosseinzadeh, Griffin, Hoang, Emily, Jha, Saurabh W., Janzen, Daryl, Jencson, Jacob E., Lundquist, Michael, Mehta, Darshana, Ravi, Aravind P., Retamal, Nicolas E. Meza, Pearson, Jeniveve, Shrestha, Manisha, Bonanos, Alceste, Howell, D. Andrew, Smith, Nathan, Farah, Joseph, Hiramatsu, Daichi, Itagaki, Koichi, McCully, Curtis, Newsome, Megan, Gonzalez, Estefania Padilla, Paraskeva, Emmanouela N., Pellegrino, Craig, Terreran, Giacomo, Haislip, Joshua, Kouprianov, Vladimir, Reichart, Daniel E.
We present photometric and spectroscopic observations of SN 2023fyq, a type Ibn supernova in the nearby galaxy NGC 4388 (D$\simeq$18~Mpc). In addition, we trace long-standing precursor emission at the position of SN 2023fyq using data from DLT40, ATL
Externí odkaz:
http://arxiv.org/abs/2405.04583
Autor:
Liakos, Alexios, Bonanos, Alceste Z., Xilouris, Emmanouil M., Koschny, Detlef, Bellas-Velidis, Ioannis, Boumis, Panagiotis, Maroussis, Athanassios, Moissl, Richard
Publikováno v:
A&A 687, A14 (2024)
We present results of the NELIOTA campaign for lunar impact flashes observed with the 1.2 m Kryoneri telescope. From August 2019 to August 2023, we report 113 validated and 70 suspected flashes. For the validated flashes, we calculate the physical pa
Externí odkaz:
http://arxiv.org/abs/2403.19613
Publikováno v:
A&A 686, A88 (2024)
The high mass-loss rates of red supergiants (RSGs) drastically affect their evolution and final fate, but their mass-loss mechanism remains poorly understood. Various empirical prescriptions scaled with luminosity have been derived in the literature,
Externí odkaz:
http://arxiv.org/abs/2401.15163
Autor:
Bonanos, A. Z., Tramper, F., de Wit, S., Christodoulou, E., Munoz-Sanchez, G., Antoniadis, K., Athanasiou, S., Maravelias, G., Yang, M., Zapartas, E.
Publikováno v:
A&A 686, A77 (2024)
The ASSESS project aims to determine the role of episodic mass-loss in the evolution of massive stars. As a first step, we construct a catalog of spectroscopically identified dusty, evolved massive stars in ten southern galaxies for which Spitzer poi
Externí odkaz:
http://arxiv.org/abs/2312.04626
Autor:
Bonanos, A. Z., Maravelias, G., Yang, M., Tramper, F., de Wit, S., Zapartas, E., Antoniadis, K., Christodoulou, E., Munoz-Sanchez, G.
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 introduce the ERC-funded ASSESS project (2018-2024), which
Externí odkaz:
http://arxiv.org/abs/2308.04891
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