Zobrazeno 1 - 3
of 3
pro vyhledávání: '"Mikolajczyk, Przemyslaw J."'
Autor:
Nagy, Zsófia, Park, Sunkyung, Ábrahám, Péter, Kóspál, Ágnes, de Miera, Fernando Cruz-Sáenz, Kun, Mária, Siwak, Michał, Szabó, Zsófia Marianna, Szilágyi, Máté, Fiorellino, Eleonora, Giannini, Teresa, Lee, Jae-Joon, Lee, Jeong-Eun, Marton, Gábor, Szabados, László, Vitali, Fabrizio, Andrzejewski, Jan, Gromadzki, Mariusz, Hodgkin, Simon, Jabłońska, Maja, Mendez, Rene A., Merc, Jaroslav, Michniewicz, Olga, Mikołajczyk, Przemysław J., Pylypenko, Uliana, Ratajczak, Milena, Wyrzykowski, Łukasz, Zejmo, Michal, Zieliński, Paweł
FU Orionis objects (FUors) are eruptive young stars, which exhibit outbursts that last from decades to a century. Due to the duration of their outbursts, and to the fact that only about two dozens of such sources are known, information on the end of
Externí odkaz:
http://arxiv.org/abs/2307.01629
Autor:
Froebrich, Dirk, Hillenbrand, Lynne A., Herbert, Carys, De, Kishalay, Eislöffel, Jochen, Campbell-White, Justyn, Kahar, Ruhee, Hambsch, Franz-Josef, Urtly, Thomas, Popowicz, Adam, Bernacki, Krzysztof, Malcher, Andrzej, Lasota, Slawomir, Fiolka, Jerzy, Jozwik-Wabik, Piotr, Dubois, Franky, Logie, Ludwig, Rau, Steve, Phillips, Mark, Fleming, George, Farfán, Rafael Gonzalez, Alfaro, Francisco C. Soldán, Nelson, Tim, Futcher, Stephen R. L., Rolfe, Samantha M., Campbell, David A., Vale, Tony, Devine, Pat, Moździerski, Dawid, Mikołajczyk, Przemysław J., Eggenstein, Heinz-Bernd, Rodriguez, Diego, Walton, Ivan L, Vanaverbeke, Siegfried, Merrikin, Barry, Öğmen, Yenal, Perez, Alex Escartin, Aimar, Mario Morales, Piehler, Georg, Dover, Lord, Patel, Aashini L., Miller, Niall, Finch, Jack, Hankins, Matt, Moore, Anna M., Travouillon, Tony, Szczepanski, Marek
This paper is one in a series reporting results from small telescope observations of variable young stars. Here, we study the repeating outbursts of three likely Be stars based on long-term optical, near-infrared, and mid-infrared photometry for all
Externí odkaz:
http://arxiv.org/abs/2302.02696
Autor:
Jiang, Chen, Wu, Tao, Feinstein, Adina D., Stassun, Keivan G., Bedding, Timothy R., Veras, Dimitri, Corsaro, Enrico, Buzasi, Derek L., Stello, Dennis, Li, Yaguang, Mathur, Savita, Garcia, Rafael A., Breton, Sylvain N., Lundkvist, Mia S., Mikolajczyk, Przemyslaw J., Gehan, Charlotte, Campante, Tiago L., Bossini, Diego, Kane, Stephen R., Ong, Jia Mian Joel, Yildiz, Mutlu, Kayhan, Cenk, Orhan, Zeynep Celik, Ortel, Sibel, Zhang, Xinyi, Cunha, Margarida S., de Moura, Bruno Lustosa, Yu, Jie, Huber, Daniel, Ou, Jian-wen, Wittenmyer, Robert A., Gizon, Laurent, Chaplin, William J.
The Transiting Exoplanet Survey Satellite (TESS) mission searches for new exoplanets. The observing strategy of TESS results in high-precision photometry of millions of stars across the sky, allowing for detailed asteroseismic studies of individual s
Externí odkaz:
http://arxiv.org/abs/2302.01102