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Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
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Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the origi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1f37637ebba59db13b7a87018e8e2c47
http://hdl.handle.net/10261/217544
http://hdl.handle.net/10261/217544
Autor:
Nicolas Peretto, M. Figueira, Alexander Men'shchikov, Ph. André, Y. Shimajiri, D. Russeil, P. Palmeirim, Nicola Schneider, Vera Konyves, Annie Zavagno, H. Roussel, Timea Csengeri, S. N. Zhang, Gary A. Fuller, Frederic Schuller, Doris Arzoumanian
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 638, pp.A7. ⟨10.1051/0004-6361/202037815⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 638, pp.A7. ⟨10.1051/0004-6361/202037815⟩
Massive stars and their associated ionized (HII) regions could play a key role in the formation and evolution of filaments that host star formation. However, the properties of filaments that interact with H regions are still poorly known. To investig
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::71224a203613f99e370d70715cc8f75c
Autor:
Natalie A. Krivova, Alexander Shapiro, Yvonne C. Unruh, N.-E. Nèmec, Sami K. Solanki, Emre Işık
Publikováno v:
Astronomy & Astrophysics
Comparing solar and stellar brightness variations is hampered by the difference in spectral passbands used in observations as well as by the possible difference in the inclination of their rotation axes from the line of sight. We calculate the rotati
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c670dd0786d3b30bce2d33f8f42b4810
http://hdl.handle.net/10044/1/80452
http://hdl.handle.net/10044/1/80452
Global magnetic fields of active solar-like stars are nowadays routinely detected with spectropolarimetric measurements and are mapped with Zeeman-Doppler imaging (ZDI). However, due to the cancellation of opposite field polarities, polarimetry captu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::52d74bad16d6114028d4819fde395228
https://aaltodoc.aalto.fi/handle/123456789/44012
https://aaltodoc.aalto.fi/handle/123456789/44012
Autor:
Eugene Semenko
Publikováno v:
EPJ Web of Conferences, Vol 240, p 05003 (2020)
A strong and stable magnetic field covering the whole surface is a landmark of chemically peculiar or CP stars. To explain the origin of mag- netic stars, several hypotheses were proposed, which depending on the mech- anism and time of formation can
Autor:
H. Ottacher, T. Kuntzer, M. Steller, Xavier Bonfils, A. García Muñoz, Don Pollacco, Ingo Walter, Gaetano Scandariato, A. Deline, Ignasi Ribas, J. Hasiba, T. Bandy, Bruno Chazelas, Yann Alibert, Luca Marafatto, Maria Bergomi, E. Hernandez, Michaël Gillon, Anders Erikson, O. Demangeon, Valerio Nascimbeni, Heike Rauer, N. Thomas, Virginie Cessa, G. Olofsson, F. Safa, R. Rohlfs, N. A. Walton, C. Broeg, Didier Queloz, C. Corral Van Damme, D. Futyan, Nicola Rando, Malcolm Fridlund, Federico Biondi, Roi Alonso, David Ehrenreich, T. Lüftinger, Stéphane Udry, László L. Kiss, K. G. Isaak, Wolfgang Baumjohann, Alexis M. S. Smith, Monika Lendl, D. Wolter, A. E. Simon, Thomas Beck, L. Malvasio, Nuno C. Santos, David Barrado, Demetrio Magrin, J. Asquier, V. Singh, Enric Palle, Damien Ségransan, Pierre F. L. Maxted, Roland Ottensamer, Gisbert Peter, M.-D. Busch, S. C. C. Barros, D. Kitzmann, Willy Benz, S. Hoyer, B. M. Morris, C. Lovis, Kevin Heng, Isabella Pagano, S. Salmon, Davide Gandolfi, Jacopo Farinato, Gy. M. Szabó, Sébastien Charnoz, Giampaolo Piotto, A. Bekkelien, Andrea Fortier, M. Sordet, A. Bonfanti, Nicolas Billot, Luca Fossati, Jacques Laskar, Francois Wildi, Szilard Csizmadia, Martin Rieder, M. Tschentscher, Valérie Van Grootel, Valentina Viotto, Vincent Bourrier, Roberto Ragazzoni, M. Beck, M. J. Hooton, F. Ratti, T. G. Wilson, T. Bárczy, L. Delrez, Daniele Piazza, A. Collier Cameron, Melvyn B. Davies, S. G. Sousa, B. O. Demory, Juan Cabrera, Alexis Brandeker, P. Guterman, M. Deleuil, A. Lecavelier des Etangs, Harald Michaelis, Matteo Munari
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Universidad de Alicante (UA)
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 643, pp.A94. ⟨10.1051/0004-6361/202038677⟩
Instituto Nacional de Técnica Aeroespacial (INTA)
Astronomy & Astrophysics, 643, A94
Astronomy & Astrophysics
instname
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Universidad de Alicante (UA)
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 643, pp.A94. ⟨10.1051/0004-6361/202038677⟩
Instituto Nacional de Técnica Aeroespacial (INTA)
Astronomy & Astrophysics, 643, A94
Astronomy & Astrophysics
Full author list: Lendl, M., Csizmadia, S., Deline, A., Fossati, L., Kitzmann, D., Heng, K., Hoyer, S., Salmon, S., Benz, W., Broeg, C., Ehrenreich, D., Fortier, A., Queloz, D., Bonfanti, A., Brandeker, A., Collier Cameron, A., Delrez, L.a,g,l, Garci
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3cbc96a49f2414c36011fda966f130a2
http://hdl.handle.net/10261/234160
http://hdl.handle.net/10261/234160
Autor:
Hector Canovas, Matías Montesinos, Simon Casassus, Valentin Christiaens, G. Cugno, Sebastián Pérez, Nuria Huélamo, Lucas A. Cieza, Alice Zurlo
Publikováno v:
Astronomy & Astrophysics, 633
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2020, 633, ⟨10.1051/0004-6361/201936891⟩
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Instituto Nacional de Técnica Aeroespacial (INTA)
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2020, 633, ⟨10.1051/0004-6361/201936891⟩
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Instituto Nacional de Técnica Aeroespacial (INTA)
Context. The mechanisms of planet formation are still under debate. We know little about how planets form, even if more than 4000 exoplanets have been detected to date. Recent investigations target the cot of newly born planets: the protoplanetary di
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c6a6bb0a6c20112a0d7f9688344f8fb5
https://hdl.handle.net/20.500.11850/397040
https://hdl.handle.net/20.500.11850/397040
Publikováno v:
EPJ Web of Conferences, Vol 240, p 05002 (2020)
We present a brief review of the recent results of photometric and spectroscopic surveys and 3-D hydrodynamic simulations of the mass- transfer for the class of oscillating mass-accreting components of Algols (oEA stars). These ground-based spectrosc
Autor:
A. P. Hatzes, D. Hintz, M. Lafarga, S. Czesla, F. F. Bauer, Ignasi Ribas, Jose A. Caballero, Erick Nagel, L. Hildebrandt, D. Montes, Ansgar Reiners, Lisa Nortmann, Andreas Quirrenbach, Jürgen H. M. M. Schmitt, Adrian Kaminski, M. Cortés-Contreras, Sandra V. Jeffers, E. N. Johnson, S. Dreizler, D. Galadí-Enríquez, Mathias Zechmeister, Birgit Fuhrmeister, M. Kürster, Pedro J. Amado, V. J. S. Béjar, P. Schöfer
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
E-Prints Complutense. Archivo Institucional de la UCM
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
Instituto Nacional de Técnica Aeroespacial (INTA)
instname
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
E-Prints Complutense. Archivo Institucional de la UCM
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
Instituto Nacional de Técnica Aeroespacial (INTA)
The He I infrared (IR) triplet at 10 830 Å is known as an activity indicator in solar-type stars and has become a primary diagnostic in exoplanetary transmission spectroscopy. He I IR lines are a tracer of the stellar extreme-ultraviolet irradiation
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fddce197ce5655fbc6c692cfc510818e
http://hdl.handle.net/10261/222716
http://hdl.handle.net/10261/222716
Autor:
M. J. Barlow, C. Agliozzo, Daniel Asmus, Patrick W. Morris, T. R. Gull, Gerd Weigelt, D. J. Hillier, W. J. de Wit, Andrea Mehner
Publikováno v:
Astronomy & Astrophysics
η Car is one of the most luminous and massive stars in our Galaxy and is the brightest mid-IR source in the sky outside our solar system. Since the late 1990s, the central source has dramatically brightened at UV and optical wavelengths. This might
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cb57681fd2088a16c1da0943fa68bc38
https://resolver.caltech.edu/CaltechAUTHORS:20191018-084050524
https://resolver.caltech.edu/CaltechAUTHORS:20191018-084050524