Zobrazeno 1 - 10
of 173
pro vyhledávání: '"general [Kuiper Belt]"'
Autor:
E. Fernández-Valenzuela, N. Morales, M. Vara-Lubiano, J. L. Ortiz, G. Benedetti-Rossi, B. Sicardy, M. Kretlow, P. Santos-Sanz, B. Morgado, D. Souami, F. Organero, L. Ana, F. Fonseca, A. Román, S. Alonso, R. Gonçalves, M. Ferreira, R. Iglesias-Marzoa, J. L. Lamadrid, A. Alvarez-Candal, M. Assafin, F. Braga-Ribas, J. I. B. Camargo, F. Colas, J. Desmars, R. Duffard, J. Lecacheux, A. R. Gomes-Júnior, F. L. Rommel, R. Vieira-Martins, C. L. Pereira, V. Casanova, A. Selva, C. Perelló, S. Mottola, S. Hellmich, J. L. Maestre, A. J. Castro-Tirado, A. Pal, J. M. Trigo-Rodriguez, W. Beisker, A. Laporta, M. Garcés, L. Escaned, M. Bretton
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2023, 669, pp.A112. ⟨10.1051/0004-6361/202243214⟩
Astronomy and Astrophysics-A&A, 2023, 669, pp.A112. ⟨10.1051/0004-6361/202243214⟩
Within our program of physical characterization of trans-Neptunian objects and centaurs, we predicted a stellar occultation by the centaur (54598) Bienor to occur on January 11, 2019, with good observability potential. We obtained high accuracy astro
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f04abb1eb2175631ceb9b5b637aab6bc
http://hdl.handle.net/10261/308511
http://hdl.handle.net/10261/308511
Akademický článek
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Do instabilities in high-multiplicity systems explain the existence of close-in white dwarf planets?
Publikováno v:
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
instname
instname
We investigate the origin of close-in planets and related phenomena orbiting white dwarfs (WDs), which are thought to originate from orbits more distant from the star. We use the planetary architectures of the 75 multiple-planet systems (four, five a
Publikováno v:
Scopus
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
Made available in DSpace on 2019-10-06T15:35:22Z (GMT). No. of bitstreams: 0 Previous issue date: 2019-04-21 The main goal of this work is to locate stable regions in the Pluto system where objects can be detected. The orbital evolution of large and
Autor:
Pierre Vernazza, Tadeusz Michalowski, Bin Yang, Matti Viikinkoski, Brian Warner, Agnieszka Kryszczyńska, Alexis Drouard, Alexander Storrs, Franck Marchis, J. Grice, François Colas, Patrick Michel, Laurent Jorda, Romain Fétick, Przemyslaw Bartczak, Arthur Vigan, Josef Ďurech, Marc Neveu, Frédéric Vachier, Julie Castillo-Rogez, Emmanuel Jehin, Michael Marsset, Josef Hanus, Nicolas Rambaux, Josselin Desmars, Mikko Kaasalainen, Marin Ferrais, Jérôme Berthier, Olivier Witasse, Philippe Lamy, Zouhair Benkhaldoun, E. Podlewska-Gaca, Fabrice Cipriani, Grzegorz Dudziński, Thierry Fusco, Raoul Behrend, Christophe Dumas, Anna Marciniak, Mirel Birlan, M. Pajuelo, Paolo Tanga, Benoit Carry, T. Santana-Ros, Mark A. Wieczorek
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, (in press)
Astronomy and Astrophysics-A&A, 2021, 650, A129 (15pp.). ⟨10.1051/0004-6361/202140342⟩
RUA. Repositorio Institucional de la Universidad de Alicante
Universidad de Alicante (UA)
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 650, A129 (15pp.). ⟨10.1051/0004-6361/202140342⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, (in press)
Astronomy and Astrophysics-A&A, 2021, 650, A129 (15pp.). ⟨10.1051/0004-6361/202140342⟩
RUA. Repositorio Institucional de la Universidad de Alicante
Universidad de Alicante (UA)
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 650, A129 (15pp.). ⟨10.1051/0004-6361/202140342⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Carri, B., et al.
[Context] Dynamical models of Solar System evolution have suggested that the so-called P- and D-type volatile-rich asteroids formed in the outer Solar System beyond Neptune's orbit and may be genetically related to the Jupiter
[Context] Dynamical models of Solar System evolution have suggested that the so-called P- and D-type volatile-rich asteroids formed in the outer Solar System beyond Neptune's orbit and may be genetically related to the Jupiter
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::aec903693a44de38f7a8bdfa34727e1b
https://hal-insu.archives-ouvertes.fr/insu-03184663/document
https://hal-insu.archives-ouvertes.fr/insu-03184663/document
Autor:
Josselin Desmars, A. Burtovoi, H. Mikuž, J. R. de Barros, Emmanuel Jehin, Marcelo Assafin, J. Fabrega Polleri, S. Sposetti, D. Herald, R. Szakats, A. R. Gomes-Júnior, Bruno Sicardy, D. W. Dunham, H. Tomioka, A. Ossola, Domenico Nardiello, F. L. Rommel, C. L. Pereira, A. Stechina, T. Hayamizu, Sohrab Rahvar, P. Sogorb, R. Vieira-Martins, Jose Luis Ortiz, Julio Camargo, J. B. Dunham, Luca Zampieri, P. Pravec, R. Komžík, J. Broughton, T. Janik, Anaëlle Maury, B. E. Morgado, P. M. Kilmartin, Pablo Santos-Sanz, G. Benedetti-Rossi, K. Hosoi, Rafael Sfair, Othon C. Winter, Nicolás Morales, D. Gault, András Pál, Y. Ueno, J. Tregloan-Reed, A. C. Gilmore, T. Carruthers, Estela Fernández-Valenzuela, P. B. Siqueira, J. Lecacheux, W. Hanna, Rhian H. Jones, Michele Fiori, Jeffrey A. Newman, Valerio Nascimbeni, Jonathan Bradshaw, K. Kitazaki, E. Pimentel, Rene Duffard, Felipe Braga-Ribas, Jan Maarten Winkel, S. Kerr, P. Nosworthy, A. Marciniak, D. Hooper, Giampiero Naletto, C. Jacques, Kamil Hornoch, Colin Snodgrass, Joseph Brimacombe
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 644, pp.A40. ⟨10.1051/0004-6361/202039054⟩
Astronomy and Astrophysics-A&A, 2020, 644, pp.A40. ⟨10.1051/0004-6361/202039054⟩
Scopus
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
Astronomy & Astrophysics
Digital.CSIC. Repositorio Institucional del CSIC
instname
Rommel, F L, Braga-Ribas, F, Desmars, J, Camargo, J I B, Ortiz, J L, Sicardy, B, Vieira-Martins, R, Assafin, M, Santos-Sanz, P, Duffard, R, Fernández-Valenzuela, E, Lecacheux, J, Morgado, B E, Benedetti-Rossi, G, Gomes-Júnior, A R, Pereira, C L, Herald, D, Hanna, W, Bradshaw, J, Morales, N, Brimacombe, J, Burtovoi, A, Carruthers, T, Barros, J R D, Fiori, M, Gilmore, A, Hooper, D, Hornoch, K, Jacques, C, Janik, T, Kerr, S, Kilmartin, P, Winkel, J M, Naletto, G, Nardiello, D, Nascimbeni, V, Newman, J, Ossola, A, Pál, A, Pimentel, E, Pravec, P, Sposetti, S, Stechina, A, Szákats, R, Ueno, Y, Zampieri, L, Broughton, J, Dunham, J B, Dunham, D W, Gault, D, Hayamizu, T, Hosoi, K, Jehin, E, Jones, R, Kitazaki, K, Komžík, R, Marciniak, A, Maury, A, Mikuž, H, Nosworthy, P, Polleri, J F, Rahvar, S, Sfair, R, Siqueira, P B, Snodgrass, C, Sogorb, P, Tomioka, H, Tregloan-Reed, J & Winter, O C 2020, ' Stellar occultations enable milliarcsecond astrometry for Trans-Neptunian objects and Centaurs ', Astronomy and Astrophysics, vol. 644, A40 . https://doi.org/10.1051/0004-6361/202039054
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 644, pp.A40. ⟨10.1051/0004-6361/202039054⟩
Astronomy and Astrophysics-A&A, 2020, 644, pp.A40. ⟨10.1051/0004-6361/202039054⟩
Scopus
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
Astronomy & Astrophysics
Digital.CSIC. Repositorio Institucional del CSIC
instname
Rommel, F L, Braga-Ribas, F, Desmars, J, Camargo, J I B, Ortiz, J L, Sicardy, B, Vieira-Martins, R, Assafin, M, Santos-Sanz, P, Duffard, R, Fernández-Valenzuela, E, Lecacheux, J, Morgado, B E, Benedetti-Rossi, G, Gomes-Júnior, A R, Pereira, C L, Herald, D, Hanna, W, Bradshaw, J, Morales, N, Brimacombe, J, Burtovoi, A, Carruthers, T, Barros, J R D, Fiori, M, Gilmore, A, Hooper, D, Hornoch, K, Jacques, C, Janik, T, Kerr, S, Kilmartin, P, Winkel, J M, Naletto, G, Nardiello, D, Nascimbeni, V, Newman, J, Ossola, A, Pál, A, Pimentel, E, Pravec, P, Sposetti, S, Stechina, A, Szákats, R, Ueno, Y, Zampieri, L, Broughton, J, Dunham, J B, Dunham, D W, Gault, D, Hayamizu, T, Hosoi, K, Jehin, E, Jones, R, Kitazaki, K, Komžík, R, Marciniak, A, Maury, A, Mikuž, H, Nosworthy, P, Polleri, J F, Rahvar, S, Sfair, R, Siqueira, P B, Snodgrass, C, Sogorb, P, Tomioka, H, Tregloan-Reed, J & Winter, O C 2020, ' Stellar occultations enable milliarcsecond astrometry for Trans-Neptunian objects and Centaurs ', Astronomy and Astrophysics, vol. 644, A40 . https://doi.org/10.1051/0004-6361/202039054
Full list of authors: Rommel, F. L.; Braga-Ribas, F.; Desmars, J.; Camargo, J. I. B.; Ortiz, J. L.; Sicardy, B.; Vieira-Martins, R.; Assafin, M.; Santos-Sanz, P.; Duffard, R.; Fernández-Valenzuela, E.; Lecacheux, J.; Morgado, B. E.; Benedetti-Rossi,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0273a2d478f1e12a33cc8509a6f8b898
http://hdl.handle.net/10261/228273
http://hdl.handle.net/10261/228273
Publikováno v:
Robinson, J, Fraser, W, Fitzsimmons, A & Lacerda, P 2020, ' Investigating Gravitational Collapse of a Pebble Cloud to form Transneptunian Binaries ', Astronomy & Astrophysics, vol. 643, A55 . https://doi.org/10.1051/0004-6361/202037456
Context. A large fraction of transneptunian objects are found in binary pairs, ~30% in the cold classical population between $a_\text{hel}$~39 and ~48 AU. Observationally, these binaries generally have components of similar size and colour. Previous
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4b5a393b2d53286339e15732c869046b
https://doi.org/10.1051/0004-6361/202037456
https://doi.org/10.1051/0004-6361/202037456
Autor:
M. H. M. Morais, Fathi Namouni
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, 2020, 493 (2), pp.2854-2871. ⟨10.1093/mnras/staa348⟩
Web of Science
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2020, 493 (2), pp.2854-2871. ⟨10.1093/mnras/staa348⟩
Web of Science
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
We apply the analytical disturbing function for arbitrary inclination derived in our previous work to characterize resonant width and libration of mean motion resonances at arbitrary inclination obtained from direct numerical simulations of the three
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::16363a6bd95bce0e36fabffffe9c3141
http://arxiv.org/abs/2002.01832
http://arxiv.org/abs/2002.01832
Autor:
G. Scarfi, T. Pribulla, J. C. Guirado, L. Buzzi, Grzegorz Dudziński, A. Farkas-Takács, L. Mazzei, E. Meza, A. Aletti, J. M. Christille, C. Perelló, L. Morrone, V. Peris, Valerio Nascimbeni, J. Lecacheux, J. M. Madiedo, Rene Duffard, F. Mancini, Bruno Sicardy, J. Alikakos, Vassilis Charmandaris, Cs. Kiss, M. Conjat, Raoul Behrend, R. Komžík, Frédéric Vachier, Martina Maestripieri, J. Skvarc, Paolo Bacci, T. G. Mueller, Domenico Nardiello, R. Iglesias-Marzoa, F. Colas, Aleksandar Cikota, András Pál, N. Paschalis, R. Szakats, A. Campo Bagatin, P. J. Gutierrez, Giacomo Succi, Pablo Santos-Sanz, A. R. Gomes-Júnior, Gábor Marton, M. Butkiewicz-Bak, E. Varga-Verebélyi, M. Masucci, Estela Fernández-Valenzuela, V. Tsamis, Victor Ali-Lagoa, Felipe Braga-Ribas, M. Alighieri, Roberto Vieira-Martins, F. Manzano, Julio Camargo, E. Dal Canto, S. Hellmich, F. Roques, A. Vecchione, A. Navarro, Stefano Mottola, A. Noschese, Albino Carbognani, F. Lavalade, Josselin Desmars, Mónica Vara-Lubiano, Nora Morales, C. Schnabel, Mauro Bachini, Kosmas Gazeas, J. M. Mari, Przemyslaw Bartczak, W. Beisker, S. Sposetti, F. Ciabattari, A. Alvarez-Candal, Stefan Cikota, J. L. Ortiz, Marcelo Assafin, A. Marciniak, G. Benedetti-Rossi, H. Mikuz
Publikováno v:
Astronomy & Astrophysics
RUA. Repositorio Institucional de la Universidad de Alicante
Universidad de Alicante (UA)
Scopus
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 639, pp.A134. ⟨10.1051/0004-6361/202038046⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy and Astrophysics-A&A, 2020, 639, pp.A134. ⟨10.1051/0004-6361/202038046⟩
RUA. Repositorio Institucional de la Universidad de Alicante
Universidad de Alicante (UA)
Scopus
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 639, pp.A134. ⟨10.1051/0004-6361/202038046⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy and Astrophysics-A&A, 2020, 639, pp.A134. ⟨10.1051/0004-6361/202038046⟩
All authors: Ortiz, J. L.; Santos-Sanz, P.; Sicardy, B.; Benedetti-Rossi, G.; Duffard, R.; Morales, N.; Braga-Ribas, F.; Fernández-Valenzuela, E.; Nascimbeni, V.; Nardiello, D.; Carbognani, A.; Buzzi, L.; Aletti, A.; Bacci, P.; Maestripieri, M.; Maz
Autor:
Adrian Brunini, María Cristina López
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 479:1392-1400
We present a semi-analytic model to evaluate the delivery of water to the habitable zone (HZ) around a solar type star carried by icy planetesimals born beyond the snow line. The model includes sublimation of ice, gas drag, and scattering by an outer