Zobrazeno 1 - 10
of 64
pro vyhledávání: '"Kanaan Samer"'
Autor:
Willson, Matthew, Kraus, Stefan, Kluska, Jacques, Monnier, John D., Cure, Michel, Sitko, Mike, Aarnio, Alicia, Ireland, Michael J., Rizzuto, Aaron, Hone, Edward, Kreplin, Alexander, Andrews, Sean, Calvet, Nuria, Espaillat, Catherine, Fukagawa, Misato, Harries, Tim J., Hinkley, Sasha, Kanaan, Samer, Muto, Takayuki, Wilner, David J.
Publikováno v:
A&A 621, A7 (2019)
V1247 Orionis harbours a pre-transitional disc with a partially cleared gap. Earlier interferometric and polarimetric observations revealed strong asymmetries both in the gap region and in the outer disc. The presence of a companion was inferred to e
Externí odkaz:
http://arxiv.org/abs/1811.06880
Autor:
Setterholm, Benjamin R., Monnier, John D., Davies, Claire L., Kreplin, Alexander, Kraus, Stefan, Baron, Fabien, Aarnio, Alicia, Berger, Jean-Philippe, Calvet, Nuria, Curé, Michel, Kanaan, Samer, Kloppenborg, Brian, Bouquin, Jean-Baptiste Le, Millan-Gabet, Rafael, Rubinstein, Adam E., Sitko, Michael L., Sturmann, Judit, Brummelaar, Theo A. ten, Touhami, Yamina
The physical processes occurring within the inner few astronomical units of proto-planetary disks surrounding Herbig Ae stars are crucial to setting the environment in which the outer planet-forming disk evolves and put critical constraints on the pr
Externí odkaz:
http://arxiv.org/abs/1811.03778
Autor:
Günther, Hans Moritz, Kraus, Stefan, Melis, Carl, Curé, Michel, Harries, Tim, Ireland, Michael, Kanaan, Samer, Poppenhaeger, Katja, Rizzuto, Aaron, Rodriguez, David, Schneider, Christian P., Sitko, Michael, Weigelt, Gerd, Willson, Matthew, Wolk, Scott
Publikováno v:
A&A 598, A82 (2017)
TYC 8241 2652 1 is a young star that showed a strong mid-infrared (mid-IR, 8-25 mu) excess in all observations before 2008 consistent with a dusty disk. Between 2008 and 2010 the mid-IR luminosity of this system dropped dramatically by at least a fac
Externí odkaz:
http://arxiv.org/abs/1611.01371
Autor:
Fernandes, Marcelo Borges, Chesneau, Olivier, Kraus, Michaela, Cidale, Lydia, Meilland, Anthony, Bendjoya, Philippe, de Souza, Armando Domiciano, Niccolini, Gilles, Andruchow, Ileana, Kanaan, Samer, Stee, Philippe, Millour, Florentin, Spang, Alain, Cure, Michel
Thanks to the high spatial resolution provided by long baseline interferometry, it is possible to understand the complex circumstellar geometry around stars with the B[e] phenomenon. These stars are composed by objects in different evolutionary stage
Externí odkaz:
http://arxiv.org/abs/1210.2782
Autor:
Meilland, Anthony, Millour, Florentin, Kanaan, Samer, Stee, Philippe, Petrov, Romain G., Hofmann, Karl-Heinz, Natta, Antonella, Perraut, Karine
Context. Classical Be stars are hot non-supergiant stars surrounded by a gaseous circumstellar disk that is responsible for the observed infrared-excess and emission lines. The phenomena involved in the disk formation still remain highly debated. Aim
Externí odkaz:
http://arxiv.org/abs/1111.2487
Autor:
Meilland, Anthony, Delaa, O., Stee, Philippe, Kanaan, Samer, Millour, Florentin, Mourard, Denis, Bonneau, Daniel, Petrov, Romain, Nardetto, Nicolas, Marcotto, Aurelie, Clausse, Jean-Michel, Perraut, Karine, Mcalister, H., Brummelaar, Theo A. Ten, Sturmann, J., Sturmann, L., Turner, N., Ridgway, S. T., Farrington, C., Goldfinger, P. J.
Classical Be stars are hot non-supergiant stars surrounded by a gaseous circumstellar disk that is responsible for the observed IR-excess and emission lines. The influence of binarity on these phenomena remains controversial. delta Sco is a binary sy
Externí odkaz:
http://arxiv.org/abs/1106.1746
Autor:
Millour, Florentin, Meilland, Anthony, Chesneau, Olivier, Stee, Philippe, Kanaan, Samer, Petrov, Romain, Mourard, Denis, Kraus, S.
Publikováno v:
A&A (2010) xxx
Context. To progress in the understanding of evolution of massive stars one needs to constrain the mass-loss and determine the phenomenon responsible for the ejection of matter an its reorganization in the circumstellar environment Aims. In order to
Externí odkaz:
http://arxiv.org/abs/1012.2957
Autor:
Kervella, Pierre, De Souza, Armando Domiciano, Kanaan, Samer, Meilland, Anthony, Spang, Alain, Stee, Philippe
Context: As is the case of several other Be stars, Achernar is surrounded by an envelope, recently detected by near-IR interferometry. Aims: We search for the signature of circumstellar emission at distances of a few stellar radii from Achernar, in t
Externí odkaz:
http://arxiv.org/abs/0812.2531
Publikováno v:
Astronomy and Astrophysics 455 (2006) 953
Aims. We report theoretical spectral energy distributions (SEDs), Br$\gamma$ line profiles and visibilities for two scenarios that can explain the disk dissipation of active hot stars an account for the transition from the Be to the B spectroscopic p
Externí odkaz:
http://arxiv.org/abs/astro-ph/0606233
Publikováno v:
Cureus.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e71acfef0ff507751c7d1814e776cb8b
https://doi.org/10.7759/cureus.38126
https://doi.org/10.7759/cureus.38126
