Zobrazeno 1 - 10
of 1 043
pro vyhledávání: '"Ercolino, A."'
Publikováno v:
A&A 685, A169 (2024)
Over the last decade, evidence has accumulated that massive stars do not typically evolve in isolation but instead follow a tumultuous journey with a companion star on their way to core collapse. While Roche-lobe overflow appears instrumental for the
Externí odkaz:
http://arxiv.org/abs/2402.12977
Autor:
Menon, Athira, Ercolino, Andrea, Urbaneja, Miguel A., Lennon, Daniel J., Herrero, Artemio, Hirai, Ryosuke, Langer, Norbert, Schootemeijer, Abel, Chatzopoulos, Emmanouil, Frank, Juhan, Shiber, Sagiv
Blue supergiants are the brightest stars in their host galaxies and yet their evolutionary status has been a long-standing problem in stellar astrophysics. In this pioneering work, we present a large sample of 59 early B-type supergiants in the Large
Externí odkaz:
http://arxiv.org/abs/2311.05581
Many supernovae (SNe) imply an interaction of the SN ejecta with matter (CSM) surrounding the progenitor star. This suggests that many massive stars may undergo various degrees of envelope stripping shortly before exploding, and produce a considerabl
Externí odkaz:
http://arxiv.org/abs/2308.01819
Autor:
Letizia Canu, Clotilde Sparano, Lara Naletto, Giuseppina De Filpo, Giulia Cantini, Elena Rapizzi, Serena Martinelli, Tonino Ercolino, Francesca Cioppi, Alessandro Fantoni, Lorenzo Zanatta, Alessandro Terreni, Massimo Mannelli, Michaela Luconi, Mario Maggi, Francesco Lotti
Publikováno v:
Frontiers in Endocrinology, Vol 14 (2024)
PurposeAdrenocortical carcinoma (ACC) is a rare and aggressive tumor. ACC male patients under adjuvant mitotane therapy (AMT) frequently develop hypogonadism, however sexual function has never been assessed in this setting. The aim of this retrospect
Externí odkaz:
https://doaj.org/article/c80ae0ff8c364ee99c9961898ea05a70
Autor:
Athira Menon, Andrea Ercolino, Miguel A. Urbaneja, Daniel J. Lennon, Artemio Herrero, Ryosuke Hirai, Norbert Langer, Abel Schootemeijer, Emmanouil Chatzopoulos, Juhan Frank, Sagiv Shiber
Publikováno v:
The Astrophysical Journal Letters, Vol 963, Iss 2, p L42 (2024)
Blue supergiants are the brightest stars in their host galaxies, and yet their evolutionary status has been a long-standing problem in stellar astrophysics. In this pioneering work, we present a large sample of 59 early B-type supergiants in the Larg
Externí odkaz:
https://doaj.org/article/5ed4309eb16e4e6db9e63bfcba502060
Autor:
Giuseppina De Filpo, Gabriele Parenti, Clotilde Sparano, Giulia Rastrelli, Elena Rapizzi, Serena Martinelli, Francesca Amore, Benedetta Badii, Prosperi Paolo, Tonino Ercolino, Massimo Mannelli, Mario Maggi, Letizia Canu
Publikováno v:
World Journal of Surgical Oncology, Vol 21, Iss 1, Pp 1-11 (2023)
Abstract Background Pheochromocytoma (PHEO) and paraganglioma (PGL) are rare neuroendocrine tumors characterized by hemodynamic instability, caused by the paroxysmal release of catecholamines. Patients may develop cardiovascular complications in the
Externí odkaz:
https://doaj.org/article/184ef3415cb54945a846afb5c663e6de
Autor:
Jenkins, James S., Díaz, Matías R., Kurtovic, Nicolás T., Espinoza, Néstor, Vines, Jose I., Rojas, Pablo A. Peña, Brahm, Rafael, Torres, Pascal, Cortés-Zuleta, Pía, Soto, Maritza G., Lopez, Eric D., King, George W., Wheatley, Peter J., Winn, Joshua N., Ciardi, David R., Ricker, George, Vanderspek, Roland, Latham, David W., Seager, Sara, Jenkins, Jon M., Beichman, Charles A., Bieryla, Allyson, Burke, Christopher J., Christiansen, Jessie L., Henze, Christopher E., Klaus, Todd C., McCauliff, Sean, Mori, Mayuko, Narita, Norio, Nishiumi, Taku, Tamura, Motohide, de Leon, Jerome Pitogo, Quinn, Samuel N., Villaseñor, Jesus Noel, Vezie, Michael, Lissauer, Jack J., Collins, Karen A., Collins, Kevin I., Isopi, Giovanni, Mallia, Franco, Ercolino, Andrea, Petrovich, Cristobal, Jordán, Andrés, Acton, Jack S., Armstrong, David J., Bayliss, Daniel, Bouchy, François, Belardi, Claudia, Bryant, Edward M., Burleigh, Matthew R., Cabrera, Juan, Casewell, Sarah L., Chaushev, Alexander, Cooke, Benjamin F., Eigmüller, Philipp, Erikson, Anders, Foxell, Emma, Gänsicke, Boris T., Gill, Samuel, Gillen, Edward, Günther, Maximilian N., Goad, Michael R., Hooton, Matthew J., Jackman, James A. G., Louden, Tom, McCormac, James, Moyano, Maximiliano, Nielsen, Louise D., Pollacco, Don, Queloz, Didier, Rauer, Heike, Raynard, Liam, Smith, Alexis M. S., Tilbrook, Rosanna H., Titz-Weider, Ruth, Turner, Oliver, Udry, Stéphane, Walker, Simon. R., Watson, Christopher A., West, Richard G., Palle, Enric, Ziegler, Carl, Law, Nicholas, Mann, Andrew W.
About one out of 200 Sun-like stars has a planet with an orbital period shorter than one day: an ultra-short-period planet (Sanchis-ojeda et al. 2014; Winn et al. 2018). All of the previously known ultra-short-period planets are either hot Jupiters,
Externí odkaz:
http://arxiv.org/abs/2009.12832
Autor:
Cloutier, Ryan, Rodriguez, Joseph E., Irwin, Jonathan, Charbonneau, David, Stassun, Keivan G., Mortier, Annelies, Latham, David W., Isaacson, Howard, Howard, Andrew W., Udry, Stéphane, Wilson, Thomas G., Watson, Christopher A., Pinamonti, Matteo, Lienhard, Florian, Giacobbe, Paolo, Guerra, Pere, Collins, Karen A., Beiryla, Allyson, Esquerdo, Gilbert A., Matthews, Elisabeth, Matson, Rachel A., Howell, Steve B., Furlan, Elise, Crossfield, Ian J. M., Winters, Jennifer G., Nava, Chantanelle, Ment, Kristo, Lopez, Eric D., Ricker, George, Vanderspek, Roland, Seager, Sara, Jenkins, Jon M., Ting, Eric B., Tenenbaum, Peter, Sozzetti, Alessandro, Sha, Lizhou, Ségransan, Damien, Schlieder, Joshua E., Sasselov, Dimitar, Roy, Arpita, Robertson, Paul, Rice, Ken, Poretti, Ennio, Piotto, Giampaolo, Phillips, David, Pepper, Joshua, Pepe, Francesco, Molinari, Emilio, Mocnik, Teo, Micela, Giuseppina, Mayor, Michel, Fiorenzano, Aldo F. Martinez, Mallia, Franco, Lubin, Jack, Lovis, Christophe, López-Morales, Mercedes, Kosiarek, Molly R., Kielkopf, John F., Kane, Stephen R., Jensen, Eric L. N., Isopi, Giovanni, Huber, Daniel, Hill, Michelle L., Harutyunyan, Avet, Gonzales, Erica, Giacalone, Steven, Ghedina, Adriano, Ercolino, Andrea, Dumusque, Xavier, Dressing, Courtney D., Damasso, Mario, Dalba, Paul A., Cosentino, Rosario, Conti, Dennis M., Colón, Knicole D., Collins, Kevin I., Cameron, Andrew Collier, Ciardi, David, Christiansen, Jessie, Chontos, Ashley, Cecconi, Massimo, Caldwell, Douglas A., Burke, Christopher, Buchhave, Lars, Beichman, Charles, Behmard, Aida, Beard, Corey, Murphy, Joseph M. Akana
Small planets on close-in orbits tend to exhibit envelope mass fractions of either effectively zero or up to a few percent depending on their size and orbital period. Models of thermally-driven atmospheric mass loss and of terrestrial planet formatio
Externí odkaz:
http://arxiv.org/abs/2004.06682
Autor:
Bluhm, P., Luque, R., Espinoza, N., Palle, E., Caballero, J. A., Dreizler, S., Livingston, J. H., Mathur, S., Quirrenbach, A., Stock, S., Van Eylen, V., Nowak, G., Lopez, E., Csizmadia, Sz., Osorio, M. R. Zapatero, Schoefer, P., Lillo-Box, J., Oshagh, M., Amado, P. J., Barrado, D., Bejar, V. J. S., Cale, B., Chaturvedi, P., Cifuentes, C., Cochran, W. D., Collins, K. A., Collins, K. I., Cortes-Contreras, M., Alonso, E. Diez, Mufti, M. El, Ercolino, A., Fridlund, M., Gaidos, E., Garcia, R. A., Gonzalez-Alvarez, E., Gonzalez-Cuesta, L., Guerra, P., Hatzes, A. P., Henning, T., Herrero, E., Hidalgo, D., Isopi, G., Jeffers, S. V., Jenkins, J. M., Jensen, E. L. N., Kabath, P., Kemmer, J., Korth, J., Kossakowski, D., Kuerster, M., Lafarga, M., Mallia, F., Montes, D., Morales, J. C., Morales-Calderon, M., Murgas, F., Narita, N., Plavchan, P., Passegger, V. M., Pedraz, S., Rauer, H., Redfield, S., Reffert, S., Reiners, A., Ribas, I., Ricker, G. R., Rodriguez-Lopez, C., Santos, A. R. G., Seager, S., Shan, Y., Schlecker, M., Schweitzer, A., Soto, M. G., Subjak, J., Tal-Or, L., Trifonov, T., Vanaverbeke, S., Vanderspek, R., Wittrock, J., Zechmeister, M., Zohrabi, F.
Publikováno v:
A&A 639, A132 (2020)
We report the confirmation of a transiting planet around the bright, inactive M0.5 V star TOI-1235 (TYC 4384-1735-1, V = 11.5 mag), whose transit signal was detected in the photometric time series of Sectors 14, 20, and 21 of the TESS space mission.
Externí odkaz:
http://arxiv.org/abs/2004.06218
Akademický článek
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