Zobrazeno 1 - 10
of 41
pro vyhledávání: '"Mauron, Nicolas"'
Autor:
Yang, Wenjin, Wu, Yuanwei, Gong, Yan, Mauron, Nicolas, Zhang, Bo, Menten, Karl M., Mai, Xiaofeng, Liu, Dejian, Li, Juan, Li, Jingjing
Studying stars that are located off the Galactic plane is important for understanding the formation history of the Milky Way. We searched for SiO masers toward off-plane O-rich asymptotic giant branch (AGB) stars from the catalog presented by Mauron
Externí odkaz:
http://arxiv.org/abs/2310.13489
Autor:
Kim, Hyosun, Lee, Ho-Gyu, Ohyama, Youichi, Kim, Ji Hoon, Scicluna, Peter, Chu, You-Hua, Mauron, Nicolas, Ueta, Toshiya
Publikováno v:
Proceedings of the International Astronomical Union, 17(S370), 78-83 (2023)
Recent abrupt changes of CW Leonis may indicate that we are witnessing the moment that the central carbon star is evolving off the Asymptotic Giant Branch (AGB) and entering into the pre-planetary nebula (PPN) phase. The recent appearance of a red co
Externí odkaz:
http://arxiv.org/abs/2308.15679
Autor:
Hambleton, Kelly M., Bianco, Federica B., Street, Rachel, Bell, Keaton, Buckley, David, Graham, Melissa, Hernitschek, Nina, Lund, Michael B., Mason, Elena, Pepper, Joshua, Prsa, Andrej, Rabus, Markus, Raiteri, Claudia M., Szabo, Robert, Szkody, Paula, Andreoni, Igor, Antoniucci, Simone, Balmaverde, Barbara, Bellm, Eric, Bonito, Rosaria, Bono, Giuseppe, Botticella, Maria Teresa, Brocato, Enzo, Bricman, Katja Bucar, Cappellaro, Enrico, Carnerero, Maria Isabel, Chornock, Ryan, Clarke, Riley, Cowperthwaite, Phil, Cucchiara, Antonino, D'Ammando, Filippo, Dage, Kristen C., Dall'Ora, Massimo, Davenport, James R. A., de Martino, Domitilla, de Somma, Giulia, Di Criscienzo, Marcella, Di Stefano, Rosanne, Drout, Maria, Fabrizio, Michele, Fiorentino, Giuliana, Gandhi, Poshak, Garofalo, Alessia, Giannini, Teresa, Gomboc, Andreja, Greggio, Laura, Hartigan, Patrick, Hundertmark, Markus, Johnson, Elizabeth, Johnson, Michael, Jurkic, Tomislav, Khakpash, Somayeh, Leccia, Silvio, Li, Xiaolong, Magurno, Davide, Malanchev, Konstantin, Marconi, Marcella, Margutti, Raffaella, Marinoni, Silvia, Mauron, Nicolas, Molinaro, Roberto, Moller, Anais, Moniez, Marc, Muraveva, Tatiana, Musella, Ilaria, Ngeow, Chow-Choong, Pastorello, Andrea, Petrecca, Vincenzo, Piranomonte, Silvia, Ragosta, Fabio, Reguitti, Andrea, Righi, Chiara, Ripepi, Vincenzo, Sandoval, Liliana Rivera, Stassun, Keivan G., Stroh, Michael, Terreran, Giacomo, Trimble, Virginia, Tsapras, Yiannis, van Velzen, Sjoert, Venuti, Laura, Vink, Jorick S.
The Vera C. Rubin Legacy Survey of Space and Time holds the potential to revolutionize time domain astrophysics, reaching completely unexplored areas of the Universe and mapping variability time scales from minutes to a decade. To prepare to maximize
Externí odkaz:
http://arxiv.org/abs/2208.04499
Autor:
Kim, Hyosun, Lee, Ho-Gyu, Ohyama, Youichi, Kim, Ji Hoon, Scicluna, Peter, Chu, You-Hua, Mauron, Nicolas, Ueta, Toshiya
Six images of IRC+10216 taken by the Hubble Space Telescope at three epochs in 2001, 2011, and 2016 are compared in the rest frame of the central carbon star. An accurate astrometry has been achieved with the help of Gaia Data Release 2. The position
Externí odkaz:
http://arxiv.org/abs/2105.05931
To investigate the asymptotic giant branch (AGB) population in the Galactic halo, we search for pulsating AGB stars at a heliocentric distance over 50kpc. Our research is based on the Catalina Southern Survey (CSS) catalogue of variables, comprising
Externí odkaz:
http://arxiv.org/abs/2104.15037
In order to construct a catalogue of oxygen-rich (noted M) asymptotic giant branch (AGB) stars in the halo, complementing those of carbon-rich (C) stars, previous lists of Miras and SRa semiregulars located in the nor thern hemisphere are merged and
Externí odkaz:
http://arxiv.org/abs/1903.12163
As part of our ongoing study of the evolved giants in the galactic halo, we consider the sample of 1286 long-period variables (LPVs) in the southern hemisphere provided by the Catalina Sky Survey experiment. These LPVs have periods P larger than 80 d
Externí odkaz:
http://arxiv.org/abs/1901.11427
Akademický článek
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IRC+10216 is the nearest carbon star with a very high mass-loss rate. The existence of a binary companion has been hinted by indirect observational evidence, such as the bipolar morphology of its nebula and a spiral-like pattern in its circumstellar
Externí odkaz:
http://arxiv.org/abs/1412.0083
Autor:
Nesci, Roberto, Gaudenzi, Silvia, Rossi, Corinne, Pezzotti, Camilla, Gigoyan, Kamo, Mauron, Nicolas
We report on the characterization of a number of AGB candidate stars identified with objective-prism plates of the Byurakan Observatory. Digitized photographic sky survey plates and recent CCD photometry have been used to improve the selection and di
Externí odkaz:
http://arxiv.org/abs/1404.3842