Zobrazeno 1 - 10
of 153
pro vyhledávání: '"Carlos Eiroa"'
Autor:
Itziar de Gregorio-Monsalvo, Attila Moór, Christine Chen, I. Rebollido, Pablo Riviere-Marichalar, Álvaro Ribas, Thomas Henning, Hector Canovas, Benjamin Montesinos, Marshall D. Perrin, Carlos Eiroa, Eva Villaver
Debris discs represent the last stages of planet formation and as such are expected to be depleted of primordial gas. Nonetheless, in the last few years the presence of cold gas has been reported in $\sim$ 20 debris discs from far-IR to (sub-)mm obse
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e94ac90f610e2ff66d1f9d6a4a23d820
http://arxiv.org/abs/2110.02308
http://arxiv.org/abs/2110.02308
Autor:
Pablo Riviere-Marichalar, I. Rebollido, A. Mora, Carlos Eiroa, Eva Villaver, Benjamin Montesinos, Ralf Launhardt, Th. Henning, Jesus Maldonado, Gwendolyn Meeus
Publikováno v:
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
instname
Biblos-e Archivo. Repositorio Institucional de la UAM
instname
Biblos-e Archivo. Repositorio Institucional de la UAM
Variable red- and blue-shifted absorption features observed in the Ca ii K line towards the A-type shell star $\phi$ Leo have been suggested by us in a previous work to be likely due to solid, comet-like bodies in the circumstellar (CS) environment.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e78a3e4c0d61f102f2d872af171acf13
Publikováno v:
The Astronomical Journal. 162:120
Most of our current understanding of the planet formation mechanism is based on the planet metallicity correlation derived mostly from solar-type stars harbouring gas-giant planets. To achieve a far more reaching grasp on the substellar formation pro
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bdcf4ffe98ec4e22769ecc8a4ffe7b07
Autor:
F. Cruz-Saenz de Miera, G. W. Wilson, Susana Lizano, Jorge A. Zavala, Alfredo Montaña, M. Chavez-Dagostino, Jonathan P. Marshall, David Sánchez-Arguelles, Iván Rodríguez-Montoya, Olga Vega, Carlos Eiroa, Min S. Yun, Emanuele Bertone, W. R. F. Dent, Grant M. Kennedy, F. P. Schloerb, Arturo I. Gómez-Ruiz, Milagros Zeballos, Jane Greaves, R. López-Valdivia, M. Olmedo, David H. Hughes, V. De la Luz, Eric E. Mamajek
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 462:2285-2294
ǫ Eridani is a nearby, young Sun-like star that hosts a ring of cool debris analogous\ud to the solar system’s Edgeworth-Kuiper belt. Early observations at (sub-)mm wave-\ud lengths gave tentative evidence of the presence of inhomogeneities in the
Autor:
René Liseau, I. Rebollido, A. Mora, Carlos Eiroa, Th. Henning, Gwendolyn Meeus, Ralf Launhardt, Jesus Maldonado, Johan Olofsson, Benjamin Montesinos, Pablo Riviere-Marichalar, Andres Carmona, A. Moór, A. Bayo, D. P. Iglesias, Eva Villaver, Gregor Rauw, Hector Canovas, Olivier Absil, C. Chen, Steve Ertel
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2020, 639, ⟨10.1051/0004-6361/201936071⟩
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
instname
Instituto Nacional de Técnica Aeroespacial (INTA)
Digital.CSIC. Repositorio Institucional del CSIC
Astronomy and Astrophysics-A&A, 2020, 639, ⟨10.1051/0004-6361/201936071⟩
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
instname
Instituto Nacional de Técnica Aeroespacial (INTA)
Digital.CSIC. Repositorio Institucional del CSIC
Context. While exoplanets are now routinely detected, the detection of small bodies in extrasolar systems remains challenging. Since the discovery of sporadic events, which are interpreted to be exocomets (falling evaporating bodies) around β Pic in
Autor:
I. Rebollido, D. Iglesias, Jonathan Smoker, Johan Olofsson, Benjamin Montesinos, Carlos Eiroa, Luca Sbordone, Amelia Bayo, Th. Henning, Zahed Wahhaj, Matthias R. Schreiber
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Debris disks are second generation dusty disks thought to be devoid of gas. However, this idea has been challenged in the last years by gas detections in some systems. We compiled a database of 301 debris disks and collected high--resolution optical
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::24ea1e4ae5095244f7b549ae690e3485
http://arxiv.org/abs/1806.10687
http://arxiv.org/abs/1806.10687
Autor:
G. Bryden, Jonathan P. Marshall, Mark C. Wyatt, David R. Ardila, Jean-Francois Lestrade, Brenda C. Matthews, Carlos Eiroa, Amaya Moro-Martin, Grant M. Kennedy
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2018, 476 (4), pp.4584-4591. ⟨10.1093/mnras/sty492⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2018, 476 (4), pp.4584-4591. ⟨10.1093/mnras/sty492⟩
We present the results of a Herschel survey of 21 late-type stars that host planets discovered by the radial velocity technique. The aims were to discover new disks in these systems and to search for any correlation between planet presence and disk p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bfb9699a0249fe1c6c2f70d389cd8672
https://hal.archives-ouvertes.fr/hal-02320508
https://hal.archives-ouvertes.fr/hal-02320508
Autor:
Amelia Bayo, Hervé Bouy, Maria Morales-Calderon, Carlos Eiroa, I. de Gregorio Monsalvo, John R. Stauffer, Nuria Huélamo, Alberto Noriega-Crespo, Pablo Riviere-Marichalar, Oscar Morata, Maria-Teresa Ruiz, Aina Palau, David Barrado
Publikováno v:
Biblos-e Archivo. Repositorio Institucional de la UAM
instname
instname
“Credit: Barrado, D. et al., A&A, 612 (2018): A79, reproduced with permission, c ESO”
Aims. The early evolutionary stage of brown dwarfs (BDs) is not very well characterized, especially during the embedded phase. Our goal is to gain insight
Aims. The early evolutionary stage of brown dwarfs (BDs) is not very well characterized, especially during the embedded phase. Our goal is to gain insight
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::07f02464522d1d7b02a35008a525c5af
https://resolver.caltech.edu/CaltechAUTHORS:20180509-111634586
https://resolver.caltech.edu/CaltechAUTHORS:20180509-111634586
Autor:
Davide Gandolfi, S. S. Brems, I. Rebollido, Jorge Prieto-Arranz, Eike W. Guenther, Juan Cabrera, P. Eigmüller, Sascha Grziwa, Carlos Eiroa, Michael Endl, Anders Erikson, Martin Pätzold, Diego Lorenzo-Oliveira, Judith Korth, Olga V. Zakhozhay, J. Saario, David Nespral, Paolo Donati, William D. Cochran, Alexis M. S. Smith, Malcolm Fridlund, Sz. Csizmadia, Oscar Barragán, Artie P. Hatzes, Hans J. Deeg, Luca Fossati, Luigi Mancini, Felice Cusano, Heike Rauer, Carina M. Persson
Publikováno v:
Biblos-e Archivo. Repositorio Institucional de la UAM
instname
Monthly Notices of the Royal Astronomical Society
NASA Astrophysics Data System
instname
Monthly Notices of the Royal Astronomical Society
NASA Astrophysics Data System
This is a pre-copyedited, author-produced PDF of an article accepted for publication in Monthly Notices of the Royal Astronomical Society following peer review. The version of record Barragán, O. et al. "K2-139 b: A low-mass warm Jupiter on a 29-d o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::45ae9d0e12cc4d1fb7c0ddb51ed1b629
https://hdl.handle.net/10486/684205
https://hdl.handle.net/10486/684205