Zobrazeno 1 - 10
of 52
pro vyhledávání: '"Ian Dobbs-Dixon"'
Publikováno v:
The Astronomical Journal, Vol 168, Iss 5, p 224 (2024)
In this work we revisit the problem of the dynamical stability of hierarchical triple systems with applications to circumbinary planetary orbits. We derive critical semimajor axes based on simulating and analyzing the dynamical behavior of 3 × 10 ^8
Externí odkaz:
https://doaj.org/article/a24995e354884b03ad3032335e505217
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 8 (2021)
Determining habitable zones in binary star systems can be a challenging task due to the combination of perturbed planetary orbits and varying stellar irradiation conditions. The concept of “dynamically informed habitable zones” allows us, neverth
Externí odkaz:
https://doaj.org/article/599cec2333774eeda2906258cbf6c1a7
Autor:
Ian Dobbs-Dixon
We present a new GCM-motivated multidimensional temperature parameterization of hot-Jupiter atmospheres that self consistently models the entire planet in 3D, accounting for both radiative and advective phenomena. Analytic formulations for the radiat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::216561efb372ddcc778fd98c70a73f6d
https://doi.org/10.5194/epsc2022-787
https://doi.org/10.5194/epsc2022-787
The dynamical excitation of asteroids due to mean motion resonant interactions with planets is enhanced when their parent star leaves the main sequence. However, numerical investigation of resonant outcomes within post-main-sequence simulations is co
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::88e1ba59024fee4dca3c09f68abe6522
Autor:
Uri Malamud, Tim Cunningham, Ian Dobbs-Dixon, Alexander J. Mustill, Nikolaos Georgakarakos, Dimitri Veras
Our knowledge of white dwarf planetary systems predominately arises from the region within a few Solar radii of the white dwarfs, where minor planets break up, form rings and discs, and accrete onto the star. The entry location, angle and speed into
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::458f2612605c073305f146a77e2d3dd3
http://arxiv.org/abs/2106.04601
http://arxiv.org/abs/2106.04601
Autor:
Jonathan J. Fortney, Michael R. Line, Luca Fossati, Heather A. Knutson, Taylor J. Bell, Nicolas B. Cowan, Kamen O. Todorov, Ian J. M. Crossfield, Kevin B. Stevenson, Patricio E. Cubillos, Robert T. Zellem, Ian Dobbs-Dixon, Drake Deming, Lisa Dang, Michael Zhang
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 489(2), 1995-2013. Oxford University Press
arXiv
arXiv
The exoplanet WASP-12b is the prototype for the emerging class of ultra-hot, Jupiter-mass exoplanets. Past models have predicted---and near ultra-violet observations have shown---that this planet is losing mass. We present an analysis of two sets of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a81347b204d1bb125b8a327a82f8d185
https://ui.adsabs.harvard.edu/abs/2019MNRAS.489.1995B/abstract
https://ui.adsabs.harvard.edu/abs/2019MNRAS.489.1995B/abstract
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 488:3818-3825
In 2010 the first planet was discovered around star HD 34445. Recently, another five planets were announced orbiting the same star. It is a rather dense multi-planet system with some of its planets having separations of fractions of an au and minimum
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::733376b7fa065f011b4541b34fd1a5db
https://doi.org/10.1093/mnras/stz1945
https://doi.org/10.1093/mnras/stz1945
Autor:
Nikolaos Georgakarakos, Thomas I. Maindl, Philip M. Winter, Samuele Crespi, Christoph Schäfer, Nader Haghighipour, Ian Dobbs-Dixon
The last phase of the formation of rocky planets is dominated by collisions among Moon- to Mars-sized planetary embryos. Simulations of this phase need to handle the difficulty of including the post-impact material without saturating the numerical in
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9b0e73939f3502b6d96feda62ec9a755
Autor:
Joseph Harrington, Michael D. Himes, Patricio E. Cubillos, Jasmina Blecic, Patricio M. Rojo, Ryan C. Challener, Nate B. Lust, M. Oliver Bowman, Sarah D. Blumenthal, Ian Dobbs-Dixon, Andrew S. D. Foster, Austin J. Foster, M. R. Green, Thomas J. Loredo, Kathleen J. McIntyre, Madison M. Stemm, David C. Wright
Publikováno v:
The Planetary Science Journal. 3:80
We present the open-source Bayesian Atmospheric Radiative Transfer (BART) retrieval package, which produces estimates and uncertainties for an atmosphere’s thermal profile and chemical abundances from observations. Several BART components are also
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f60d39feab9ab3f088cb8abe5d7b6d78
https://doi.org/10.3847/psj/ac3513
https://doi.org/10.3847/psj/ac3513
Autor:
Jasmina Blecic, Joseph Harrington, Patricio E. Cubillos, M. Oliver Bowman, Patricio M. Rojo, Madison Stemm, Ryan C. Challener, Michael D. Himes, Austin J. Foster, Ian Dobbs-Dixon, Andrew S. D. Foster, Nathaniel B. Lust, Sarah D. Blumenthal, Dylan Bruce, Thomas J. Loredo
Publikováno v:
The Planetary Science Journal. 3:82
This and companion papers by Harrington et al. and Cubillos et al. describe an open-source retrieval framework, Bayesian Atmospheric Radiative Transfer (BART), available to the community under the reproducible-research license via https://github.com/
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::279fc1d410c164c7c6a9fd3f0b08ef1b
https://doi.org/10.3847/psj/ac3515
https://doi.org/10.3847/psj/ac3515