Zobrazeno 1 - 10
of 130
pro vyhledávání: '"Muratore, A. F."'
Autor:
Lloyd, E. Caitlin, Foerde, Karin E., Muratore, Alexandra F., Aw, Natalie, Semanek, David, Steinglass, Joanna E., Posner, Jonathan
Publikováno v:
In Biological Psychiatry: Cognitive Neuroscience and Neuroimaging August 2023 8(8):864-873
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Muratore, Alexandra F., Attia, Evelyn
Publikováno v:
In Clinical Therapeutics January 2021 43(1):85-94
Autor:
Muratore, M. F., Kraus, M., Oksala, M. E., Arias, M. L., Cidale, L., Fernandes, M. Borges, Liermann, A.
The evolutionary phase of B[e] stars is difficult to establish due to the uncertainties in their fundamental parameters. For instance, possible classifications for the Galactic B[e] star MWC 137 include pre-main-sequence and post-main-sequence phases
Externí odkaz:
http://arxiv.org/abs/1409.7550
Massive evolved stars in transition phases, such as Luminous Blue Variables (LBVs), B[e] Supergiants (B[e]SGs), and Yellow Hypergiants (YHGs), are not well understood, and yet crucial steps in determining accurate stellar and galactic evolution model
Externí odkaz:
http://arxiv.org/abs/1308.2103
Autor:
Muratore, M. F., de Wit, W. J., Kraus, M., Aret, A., Cidale, L. S., Fernandes, M. Borges, Oudmaijer, R. D., Wheelwright, H. E.
Publikováno v:
ASP Conference Series, Vol. 464, 2012, p.67
We are investigating the circumstellar material for a sample of B[e] stars using high spectral resolution data taken in the optical and near-infrared regions with ESO/FEROS and ESO/CRIRES spectrographs, respectively. B[e] stars are surrounded by dens
Externí odkaz:
http://arxiv.org/abs/1212.4798
Autor:
Espel-Huynh, Hallie M., Muratore, Alexandra F., Virzi, Nicole, Brooks, Gayle, Zandberg, Laurie J.
Publikováno v:
In Eating Behaviors August 2019 34
Autor:
Evans, Brittney C., Murray, Helen B., Muratore, Alexandra F., Lantz, Elin L., Juarascio, Adrienne S.
Publikováno v:
In Cognitive and Behavioral Practice May 2019 26(2):395-410
Autor:
Oksala, M. E., Kraus, M., Arias, M. L., Fernandes, M. Borges, Cidale, L., Muratore, M. F., Cure, M.
Molecular emission has been detected in several Magellanic Cloud B[e] supergiants. In this Letter, we report on the detection of CO band head emission in the B[e] supergiant LHA 115-S 65, and present a K-band near-infrared spectrum obtained with the
Externí odkaz:
http://arxiv.org/abs/1207.6294
The disc formation mechanism of B[e] supergiants is one of the puzzling phenomena in massive star evolution. Rapid stellar rotation seems to play an important role for the non-spherically symmetric mass-loss leading to a high-density disc or ring-lik
Externí odkaz:
http://arxiv.org/abs/1203.6808