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pro vyhledávání: '"Alan P. Boss"'
Autor:
Alan P. Boss
Publikováno v:
The Astrophysical Journal, Vol 969, Iss 2, p 157 (2024)
Exoplanet demographics are sufficiently advanced to provide important constraints on theories of planet formation. While core and pebble accretion are preferred for rocky and icy planets, there appears to be a need for gas disk gravitational instabil
Externí odkaz:
https://doaj.org/article/ea0ad19f1f98466b9ed6f07e752502f3
Autor:
Alan P. Boss, Shubham Kanodia
Publikováno v:
The Astrophysical Journal, Vol 956, Iss 1, p 4 (2023)
Recent discoveries of gas giant exoplanets around M-dwarfs from transiting and radial velocity surveys are difficult to explain with core-accretion models. We present here a homogeneous suite of 162 models of gravitationally unstable gaseous disks. T
Externí odkaz:
https://doaj.org/article/0f5be9fd017247ec9b782799a6bd46a9
Autor:
Alan P. Boss
Publikováno v:
The Astrophysical Journal, Vol 943, Iss 2, p 101 (2023)
Protoplanets formed in a marginally gravitationally unstable (MGU) disk by either core accretion or disk instability will be subject to dynamical interactions with massive spiral arms, possibly resulting in inward or outward orbital migration, merger
Externí odkaz:
https://doaj.org/article/2dc3f9acb54945af927011bb86920bf6
Autor:
R. Paul Butler, Mark W. Phillips, Hugh R. A. Jones, Alan P. Boss, J. Burt, Bradford P. Holden, Steven S. Vogt, Rebecca Oppenheimer, Fabo Feng
To fully constrain the orbits of low mass circumstellar companions, we conduct combined analyses of the radial velocity data as well as the Gaia and Hipparcos astrometric data for eight nearby systems. Our study shows that companion-induced position
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::723ca2695b47a8d8a40024f951f90000
http://arxiv.org/abs/2107.14056
http://arxiv.org/abs/2107.14056
Autor:
Alan P. Boss
Publikováno v:
The Astrophysical Journal. 933:1
Cook et al. (2021) found that iron meteorites have an initial abundance ratio of the short-lived isotope $^{60}$Fe to the stable isotope $^{56}$Fe of $^{60}$Fe/$^{56}$Fe $\sim$ $(6.4 \pm 2.0) \times 10^{-7}$. This appears to require the injection of
Autor:
Alan P. Boss
Observations support the hypothesis that gas disk gravitational instability might explain the formation of massive or wide-orbit gas giant exoplanets. The situation with regard to Jupiter-mass exoplanets orbiting within $\sim$ 20 au is more uncertain
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::76881234b06cd43e35d061a659f78631
http://arxiv.org/abs/2103.02566
http://arxiv.org/abs/2103.02566
Autor:
Alan P. Boss
Publikováno v:
The Astrophysical Journal. 923:93
While collisional accumulation is nearly universally accepted as the formation mechanism of rock and ice worlds, the situation regarding gas giant planet formation is more nuanced. Gas accretion by solid cores formed by collisional accumulation is th
Autor:
Savita Mathur, Daniel Huber, Jennifer R. Campbell, Megan Shabram, Janice Voss, Jeffrey L. Coughlin, Guillermo Torres, Edward W. Dunham, Bruce D. Clarke, Laurance R. Doyle, Susan E. Mullally, Alan P. Boss, John Troeltzsch, Michael R. Haas, Jeffrey Van Cleve, Andrej Prsa, D. T. Sanderfer, Jeffrey C. Smith, Steve Bryson, Lauren M. Weiss, Christopher E. Henze, William F. Welsh, Elisa V. Quintana, Timothy D. Morton, Avi Shporer, Ravi Kumar Kopparapu, Fergal Mullally, Andrea K. Dupree, Jeffery J. Kolodziejczak, Joseph Catanzarite, Eric B. Ford, Solange V. Ramirez, Forrest R. Girouard, Michael Endl, Dimitar Sasselov, Christopher K. Middour, Travis A. Berger, William D. Cochran, Jørgen Christensen-Dalsgaard, Jessie L. Dotson, James L. Fanson, Natalie M. Batalha, Alan Gould, Christopher Allen, K. Larson, Jie Li, Jon M. Jenkins, Jason H. Steffen, Thomas N. Gautier, John C. Geary, Hema Chandrasekaran, Shawn Seader, Douglas A. Caldwell, Maura Fujieh, Lars A. Buchhave, Victor Silva Aguirre, Robert L. Morris, William J. Borucki, Joseph D. Twicken, David R. Ciardi, David W. Latham, Ronald L. Gilliland, Michelle Kunimoto, Steve B. Howell, Soren Meibom, Hans Kjeldsen, Andrew W. Howard, Khadeejah A. Zamudio, Darin Ragozzine, B. Wohler, William J. Chaplin, Jessie L. Christiansen, D. Pletcher, Samuel N. Quinn, Roger C. Hunter, Matthew J. Holman, Martin Still, Christopher J. Burke, David G. Koch, Geert Barentsen, Eduardo Seperuelo Duarte, Akm Kamal Uddin
Publikováno v:
Bryson, S, Kunimoto, M, Kopparapu, R K, Coughlin, J L, Borucki, W J, Koch, D, Aguirre, V S, Allen, C, Barentsen, G, Batalha, N M, Berger, T, Boss, A, Buchhave, L A, Burke, C J, Caldwell, D A, Campbell, J R, Catanzarite, J, Chandrasekaran, H, Chaplin, W J, Christiansen, J L, Christensen-Dalsgaard, J R, Ciardi, D R, Clarke, B D, Cochran, W D, Dotson, J L, Doyle, L R, Duarte, E S, Dunham, E W, Dupree, A K, Endl, M, Fanson, J L, Ford, E B, Fujieh, M, Gautier, T N, Geary, J C, Gilliland, R L, Girouard, F R, Gould, A, Haas, M R, Henze, C E, Holman, M J, Howard, A W, Howell, S B, Huber, D, Hunter, R C, Jenkins, J M, Kjeldsen, H, Kolodziejczak, J, Larson, K, Latham, D W, Li, J, Mathur, S, Meibom, S R, Middour, C, Morris, R L, Morton, T D, Mullally, F, Mullally, S E, Pletcher, D, Prsa, A, Quinn, S N, Quintana, E V, Ragozzine, D, Ramirez, S V, Sanderfer, D T, Sasselov, D, Seader, S E, Shabram, M, Shporer, A, Smith, J C, Steffen, J H, Still, M, Torres, G, Troeltzsch, J, Twicken, J D, Uddin, A K, Van Cleve, J E, Voss, J, Weiss, L M, Welsh, W F, Wohler, B & Zamudio, K A 2021, ' The Occurrence of Rocky Habitable-zone Planets around Solar-like Stars from Kepler Data ', Astronomical Journal, vol. 161, no. 1, 36 . https://doi.org/10.3847/1538-3881/abc418
Bryson, S, Kunimoto, M, Kopparapu, R K, Coughlin, J L, Borucki, W J, Koch, D, Aguirre, V S, Allen, C, Barentsen, G, Batalha, N M, Berger, T, Boss, A, Buchhave, L A, Burke, C J, Caldwell, D A, Campbell, J R, Catanzarite, J, Chandrasekaran, H, Chaplin, W J, Christiansen, J L, Christensen-Dalsgaard, J, Ciardi, D R, Clarke, B D, Cochran, W D, Dotson, J L, Doyle, L R, Duarte, E S, Dunham, E W, Dupree, A K, Endl, M, Fanson, J L, Ford, E B, Fujieh, M, III, T N G, Geary, J C, Gilliland, R L, Girouard, F R, Gould, A, Haas, M R, Henze, C E, Holman, M J, Howard, A W, Howell, S B, Huber, D, Hunter, R C, Jenkins, J M, Kjeldsen, H, Kolodziejczak, J, Larson, K, Latham, D W, Li, J, Mathur, S, Meibom, S, Middour, C, Morris, R L, Morton, T D, Mullally, F, Mullally, S E, Pletcher, D, Prsa, A, Quinn, S N, Quintana, E V, Ragozzine, D, Ramirez, S V, Sanderfer, D T, Sasselov, D, Seader, S E, Shabram, M, Shporer, A, Smith, J C, Steffen, J H, Still, M, Torres, G, Troeltzsch, J, Twicken, J D, Uddin, A K, Cleve, J E V, Voss, J, Weiss, L M, Welsh, W F, Wohler, B & Zamudio, K A 2021, ' The Occurrence of Rocky Habitable-zone Planets around Solar-like Stars from Kepler Data ', Astronomical Journal, vol. 161, no. 1, 36 . https://doi.org/10.3847/1538-3881/abc418
Bryson, S, Kunimoto, M, Kopparapu, R K, Coughlin, J L, Borucki, W J, Koch, D, Aguirre, V S, Allen, C, Barentsen, G, Batalha, N M, Berger, T, Boss, A, Buchhave, L A, Burke, C J, Caldwell, D A, Campbell, J R, Catanzarite, J, Chandrasekaran, H, Chaplin, W J, Christiansen, J L, Christensen-Dalsgaard, J, Ciardi, D R, Clarke, B D, Cochran, W D, Dotson, J L, Doyle, L R, Duarte, E S, Dunham, E W, Dupree, A K, Endl, M, Fanson, J L, Ford, E B, Fujieh, M, III, T N G, Geary, J C, Gilliland, R L, Girouard, F R, Gould, A, Haas, M R, Henze, C E, Holman, M J, Howard, A W, Howell, S B, Huber, D, Hunter, R C, Jenkins, J M, Kjeldsen, H, Kolodziejczak, J, Larson, K, Latham, D W, Li, J, Mathur, S, Meibom, S, Middour, C, Morris, R L, Morton, T D, Mullally, F, Mullally, S E, Pletcher, D, Prsa, A, Quinn, S N, Quintana, E V, Ragozzine, D, Ramirez, S V, Sanderfer, D T, Sasselov, D, Seader, S E, Shabram, M, Shporer, A, Smith, J C, Steffen, J H, Still, M, Torres, G, Troeltzsch, J, Twicken, J D, Uddin, A K, Cleve, J E V, Voss, J, Weiss, L M, Welsh, W F, Wohler, B & Zamudio, K A 2021, ' The Occurrence of Rocky Habitable-zone Planets around Solar-like Stars from Kepler Data ', Astronomical Journal, vol. 161, no. 1, 36 . https://doi.org/10.3847/1538-3881/abc418
We present occurrence rates for rocky planets in the habitable zones (HZ) of main-sequence dwarf stars based on the Kepler DR25 planet candidate catalog and Gaia-based stellar properties. We provide the first analysis in terms of star-dependent inste
Publikováno v:
The Astrophysical Journal. 901:81
Solar-type young stellar objects undergo periodic, energetic outbursts that appear to be the result of enhanced mass accretion driven by the gravitational instability of their disks. Such FU Orionis outbursts may have profound consequences for the ea
Autor:
Alan P. Boss
Cosmochemical evaluations of the initial meteoritical abundance of the short-lived radioisotope (SLRI) $^{26}$Al have remained fairly constant since 1976, while estimates for the initial abundance of the SLRI $^{60}$Fe have varied widely recently. At
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5f5a2014120e7dc3d9955d88c37f5fba
http://arxiv.org/abs/1811.05033
http://arxiv.org/abs/1811.05033