Zobrazeno 1 - 10
of 100
pro vyhledávání: '"Elvira Covino"'
Autor:
Stavro L. Ivanovski, Fabiola Antonietta Gerosa, Diego Turrini, Maria Teresa Capria, Juan Manuel Alcala, Vincenzo Della Corte, Elvira Covino, Marco Fulle, Giovanni Vladilo, Laura Silva, Davide Perna
Introduction Recent high-resolution ALMA observations of protoplanetary disks have raised interest in the study of solid bodies in disks at different scales, from sub-micrometric grains up to solid bodies hundreds of meters in size, for which dynamic
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::fc52790718328e497260fd12ff942107
https://doi.org/10.5194/epsc2021-809
https://doi.org/10.5194/epsc2021-809
Autor:
J. Eislöffel, J. Campbell-White, Lynne A. Hillenbrand, I. Mendigutía, J. Alonso-Santiago, Davide Fedele, P. McGinnis, Ágnes Kóspál, Antonio Frasca, T. Thanathibodee, P. C. Schneider, Ł. Tychoniec, Sylvie Cabrit, M. Siwak, M. Koutoulaki, E. Sanchis, F. M. Walter, Giacomo Beccari, Andrea Banzatti, A. Sicilia-Aguilar, M. Gangi, Giovanni P. Rosotti, Myriam Benisty, H. M. J. Boffin, G. A. J. Hussain, C. Ginski, N. Arulanantham, S. Antoniucci, G. J. Herczeg, Jonathan Williams, C. Briceno, K. Maucó, Hans Moritz Günther, J. M. Alcalá, L. Venuti, M. M. James, Anna Miotello, R. Garcia Lopez, G. Zsidi, William J. Fischer, Nuria Calvet, Beate Stelzer, Péter Ábrahám, Elisabetta Rigliaco, Giuseppe Lodato, B. Ercolano, R. Mentel, Francesca Bacciotti, Elvira Covino, Teresa Giannini, J. Erkal, Rene D. Oudmaijer, Leonardo Testi, S. Facchini, Min Fang, A. Caratti o Garatti, Katia Biazzo, Lee Hartmann, E. Fiorellino, Jacco Vink, J. F. Gameiro, Jesús Hernández, K. Grankin, Carlo F. Manara, Massimo Robberto, Lorenzo Spina, Catherine Dougados, Catherine Espaillat, Deirdre Coffey, Jerome Bouvier, Brunella Nisini
Publikováno v:
Astronomy & Astrophysics, 650:A196. EDP Sciences
Astronomy & Astrophysics
Astronomy & Astrophysics, 650, 1-46
Astronomy & Astrophysics
Astronomy & Astrophysics, 650, 1-46
The evolution of young stars and disks is driven by the interplay of several processes, notably accretion and ejection of material. Critical to correctly describe the conditions of planet formation, these processes are best probed spectroscopically.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::35709f6cd6d689d6db8a99b1cda4657c
https://dare.uva.nl/personal/pure/en/publications/penellope-the-eso-data-legacy-program-to-complement-the-hubble-uv-legacy-library-of-young-stars-ullyses-i(a06504a4-ee20-4ed8-a2b9-d1cb39621bfc).html
https://dare.uva.nl/personal/pure/en/publications/penellope-the-eso-data-legacy-program-to-complement-the-hubble-uv-legacy-library-of-young-stars-ullyses-i(a06504a4-ee20-4ed8-a2b9-d1cb39621bfc).html
Autor:
Juan M. Alcalá, Michal Siwak, Péter Ábrahám, L. Venuti, Frederick M. Walter, M. Gangi, J. Alonso-Santiago, Elvira Covino, H. M. J. Boffin, Antonio Frasca, Evelyne Alecian, Ágnes Kóspál, Sylvie Cabrit, K. N. Grankin, Gregory J. Herczeg, Min Fang, Carlo F. Manara
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, In press
HAL
Astronomy & Astrophysics
Astronomy and Astrophysics-A&A, EDP Sciences, In press
HAL
Astronomy & Astrophysics
We present results of our study of the close pre-main sequence spectroscopic binary CVSO 104 in Ori OB1, based on data obtained within the PENELLOPE legacy program. We derive, for the first time, the orbital elements of the system and the stellar par
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7f65e74afd8b6d10241d550b8368c1c8
https://hal.archives-ouvertes.fr/hal-03428894/file/2109.06305.pdf
https://hal.archives-ouvertes.fr/hal-03428894/file/2109.06305.pdf
Autor:
Andrea Tozzi, Rosario Cosentino, Avet Harutyunyan, Antonio Maggio, Andrea Bignamini, Aldo S. Bonomo, Valerio Nascimbeni, Luca Malavolta, Katia Biazzo, Isabella Pagano, Gloria Guilluy, Serena Benatti, Matteo Brogi, Emilio Molinari, F. Borsa, Daniela Fantinel, Mario Damasso, Marco Pedani, Adriano Ghedina, Giuseppe Leto, Paolo Giacobbe, Patricio E. Cubillos, Nicoletta Sanna, Sergei N. Yurchenko, Giampaolo Piotto, Marcello Lodi, Gaetano Scandariato, Luca Fossati, Alessandro Sozzetti, Giuseppina Micela, Siddharth Gandhi, Riccardo Claudi, Silvano Desidera, Aldo F. M. Fiorenzano, Elvira Covino, Antonino F. Lanza, Ennio Poretti, Monica Rainer, Jesus Maldonado, Lorenzo Pino, A. Galli, Katy L. Chubb, Ilaria Carleo
The atmospheres of gaseous giant exoplanets orbiting close to their parent stars (hot Jupiters) have been probed for nearly two decades. They allow us to investigate the chemical and physical properties of planetary atmospheres under extreme irradiat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::688682a274d886da6b93695ddf60cf07
Autor:
J. I. González Hernández, Matteo Pinamonti, M. Perger, R. Zanmar Sanchez, Antonio Maggio, Isabella Pagano, E. González-Álvarez, Andrea Bignamini, Jorge Maldonado, Rafael Rebolo, Alessandro Sozzetti, Giuseppina Micela, Giuseppe Leto, L. Affer, Paolo Giacobbe, B. Toledo-Padrón, Ennio Poretti, A. Petralia, Ignasi Ribas, Elvira Covino, Antonino F. Lanza, A. Suárez Mascareño, Mario Damasso, Gaetano Scandariato
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Universitat Pompeu Fabra
instname
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Universitat Pompeu Fabra
[Context] The high number of super-Earth and Earth-like planets in the habitable zone detected around M-dwarf stars in recent years has revealed these stellar objects to be the key to planetary radial velocity (RV) searches. [Aims] Using the HARPS-N
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::27eba3a275b19135565b25c487488fb1
http://hdl.handle.net/10261/257744
http://hdl.handle.net/10261/257744
Autor:
Monica Rainer, Rosario Cosentino, Ernesto Oliva, Katia Biazzo, Marco Pedani, Raffaele Gratton, Lorenzo Pino, Antonio Maggio, Emilio Molinari, Jesus Maldonado, Giampaolo Piotto, Riccardo Claudi, G. Frustagli, A. F. Martinez Fiorenzano, N. Buchschacher, Giuseppina Micela, Matteo Brogi, Luigi Mancini, Marcello Lodi, Adriano Ghedina, Gaetano Scandariato, M. Gonzalez, Marco Molinaro, Domenico Nardiello, Ilaria Carleo, Elvira Covino, Alessandro Sozzetti, F. Borsa, Antonino F. Lanza, Ennio Poretti, Giuseppe Leto, Aldo S. Bonomo, Isabella Pagano
Transiting ultra-hot Jupiters are ideal candidates to study the exoplanet atmospheres and their dynamics, particularly by means of high-resolution, high signal-to-noise ratio spectra. One such object is KELT-20b, orbiting the fast rotating A2-type st
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4b2144f12a9875d452ca60c07a9ad900
http://hdl.handle.net/11577/3397716
http://hdl.handle.net/11577/3397716
Autor:
Elisabetta Rigliaco, Antonio Frasca, C. Lazzoni, Gael Chauvin, Silvano Desidera, F. Z. Majidi, Joshua E. Schlieder, Mickael Bonnefoy, Dino Mesa, Juan M. Alcalá, Carlo F. Manara, Elvira Covino, Arthur Vigan, Raffaele Gratton, Riccardo Claudi, Maud Langlois, Valentina D'Orazi
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 635, pp.L1. ⟨10.1051/0004-6361/201937309⟩
Astronomy and Astrophysics-A&A, 2020, 635, pp.L1. ⟨10.1051/0004-6361/201937309⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 635, pp.L1. ⟨10.1051/0004-6361/201937309⟩
Astronomy and Astrophysics-A&A, 2020, 635, pp.L1. ⟨10.1051/0004-6361/201937309⟩
Substellar companions at wide separation around stars hosting planets or brown dwarfs (BDs) yet close enough for their formation in the circumstellar disc are of special interest. In this letter we report the discovery of a wide (projected separation
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3c901c969ee38d80c088f02754acaaae
https://hal.archives-ouvertes.fr/hal-02899003/document
https://hal.archives-ouvertes.fr/hal-02899003/document
Autor:
Marcello Lodi, A. F. Lanza, Andrea Bignamini, M. Sozzi, Gaetano Scandariato, C. Riverol, Jesus Maldonado, Luca Malavolta, Giuseppe Leto, R. G. Gratton, Massimo Cecconi, Katia Biazzo, Carlo Baffa, Riccardo Claudi, G. Falcini, N. Buchschacher, Marco Pedani, Elisabetta Giani, Silvano Desidera, Concepción Iglesias González, H. Perez Ventura, Luigi Mancini, Daniela Fantinel, Antonio Maggio, Salvo Scuderi, Ennio Poretti, Ulf Seemann, Andrea Tozzi, Matthias Mallonn, José Guerra, A. Galli, Giuseppina Micela, E. Alei, Valerio Nascimbeni, Avet Harutyunyan, Matteo Pinamonti, G. Frustagli, Aldo S. Bonomo, Monica Rainer, Alfio Puglisi, Aldo F. M. Fiorenzano, Livia Origlia, Serena Benatti, Alessandro Sozzetti, Isabella Pagano, Andrea Baruffolo, Adriano Ghedina, Paolo Giacobbe, M. Gonzalez, Ernesto Oliva, Ilaria Carleo, Francesca Ghinassi, Rosario Cosentino, Elvira Covino, M. Esposito, N. Hernandez, Giampaolo Piotto, M. Hernandez Diaz, Luca Fini, J. San Juan, Seth Redfield, M. Iuzzolino, Nicoletta Sanna, L. Riverol, Laura Affer, Francesco Borsa, Emilio Molinari, Mario Damasso, E. González-Álvarez, V. Billotti
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Instituto Nacional de Técnica Aeroespacial (INTA)
instname
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Instituto Nacional de Técnica Aeroespacial (INTA)
Context. The existence of hot Jupiters is still not well understood. Two main channels are thought to be responsible for their current location: a smooth planet migration through the protoplanetary disk or the circularization of an initial highly ecc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e7afd36d2b01747b9a280585ac928276
http://hdl.handle.net/2108/250712
http://hdl.handle.net/2108/250712
Autor:
Andrea Bignamini, Katia Biazzo, N. Hernandez, Giampaolo Piotto, G. Falcini, Jesus Maldonado, Antonio Maggio, Vincent Bourrier, Massimo Cecconi, Giuseppina Micela, Emilio Molinari, A. F. Lanza, Gaetano Scandariato, Riccardo Claudi, G. Frustagli, Marco Pedani, José Guerra, Andrea Baruffolo, A. F. Martinez Fiorenzano, Avet Harutyunyan, Carlo Baffa, Rosario Cosentino, Laura Affer, Silvano Desidera, Walter Boschin, Monica Rainer, Lorenzo Pino, Valerio Nascimbeni, Ennio Poretti, Serena Benatti, Alessandro Sozzetti, M. Esposito, E. González-Álvarez, Isabella Pagano, Ilaria Carleo, Matteo Brogi, Adriano Ghedina, Paolo Giacobbe, Luca Malavolta, Giuseppe Leto, Aldo S. Bonomo, Ansgar Reiners, Luigi Mancini, Luca Fossati, M. S. Giampapa, Elvira Covino, Vincenzo Andretta, Mario Damasso, G. Bruno, G. Guilluy, Francesco Borsa
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Instituto Nacional de Técnica Aeroespacial (INTA)
Astronomy & Astrophysics
instname
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Instituto Nacional de Técnica Aeroespacial (INTA)
Astronomy & Astrophysics
Exoplanets orbiting very close to their host star are strongly irradiated. This can lead the upper atmospheric layers to expand and evaporate into space. The metastable helium (HeI) triplet at 1083.3nm has recently been shown to be a powerful diagnos
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::824c39fe36377e868373e4dce80b3cb7
http://hdl.handle.net/10261/234369
http://hdl.handle.net/10261/234369
Autor:
Jesus Maldonado, L. Malavolta, Monica Rainer, Francesco Borsa, G. Bruno, A. F. Martinez Fiorenzano, Valerio Nascimbeni, Marcello Lodi, A. F. Lanza, Marco Molinaro, Gaetano Scandariato, Ilaria Carleo, Riccardo Claudi, Giuseppina Micela, Marco Pedani, Matteo Brogi, Andrea Bignamini, Avet Harutyunyan, Elvira Covino, Giuseppe Leto, M. Gonzalez, Katia Biazzo, R. G. Gratton, Luigi Mancini, Francesco Marzari, Rosario Cosentino, Laura Affer, Cristina Knapic, Mario Damasso, M. P. Di Mauro, G. Piotto, G. Frustagli, Domenico Nardiello, Silvano Desidera, Isabella Pagano, Serena Benatti, Alessandro Sozzetti, Ennio Poretti, D. Barbato, Aldo S. Bonomo, Antonio Maggio, Paolo Giacobbe, Matteo Pinamonti, Emilio Molinari
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2020, 639, ⟨10.1051/0004-6361/202037939⟩
Astronomy and Astrophysics-A&A, 2020, 639, ⟨10.1051/0004-6361/202037939⟩
In the framework of the Global Architecture of Planetary Systems (GAPS) project we collected more than 300 spectra with HARPS-N at the TNG for the bright G9V star HD164922. This target is known to host one gas giant planet in a wide orbit (Pb~1200 da
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::da69c8cee3d7d2354e2121e45600c863
http://hdl.handle.net/2108/257835
http://hdl.handle.net/2108/257835