Zobrazeno 1 - 10
of 44
pro vyhledávání: '"Rafikov, RR"'
Autor:
Rafikov, RR
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 519:5607-5622
Resolved observations of debris discs can be used to derive radial profiles of Azimuthally-averaged Surface Density (ASD), which carries important information about the disc structure even in presence of non-axisymmetric features and has improved sig
Autor:
Rafikov, RR, Cimerman, NP
High-resolution sub-mm observations of some protoplanetary discs reveal non-asixymmetric features, which can often be interpreted as dust concentrations in vortices that form at the edges of gaps carved out by the embedded planets. We use recent resu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::56c17443a959a0934eb80eaf22633db8
http://arxiv.org/abs/2301.01789
http://arxiv.org/abs/2301.01789
Autor:
Cimerman, NP, Rafikov, RR
Young planets embedded in protoplanetary discs (PPDs) excite spiral density waves, which propagate, shock and deposit angular momentum in the disc. This results in gap opening around the planetary orbit, even for low (sub-thermal) mass planets, provi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::26d45c75a2ec0379295d996b275a563d
https://www.repository.cam.ac.uk/handle/1810/347075
https://www.repository.cam.ac.uk/handle/1810/347075
Autor:
Hamilton, C, Rafikov, RR
The dozens of compact object mergers detected by LIGO/Virgo raise a key theoretical question: how do initially wide binaries shrink sufficiently quickly that they are able to merge via gravitational wave (GW) radiation within a Hubble time? One promi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2c771eb1ed55861f631e7efd5fa0acc3
https://www.repository.cam.ac.uk/handle/1810/342806
https://www.repository.cam.ac.uk/handle/1810/342806
Autor:
Rafikov, RR
Discovery of the first interstellar asteroid (ISA) - 1I/2017 'Oumuamua - raised a number of questions regarding its origin. Many of them relate to its lack of cometary activity, suggesting refractory composition of 'Oumuamua. Here we explore the poss
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______109::84d3d03db2fd041c391b154aaf9b0486
https://www.repository.cam.ac.uk/handle/1810/289293
https://www.repository.cam.ac.uk/handle/1810/289293
Autor:
Hamilton, C, Rafikov, RR
Publikováno v:
The Astrophysical Journal. 881:L13
The detections of gravitational waves produced in mergers of binary black holes (BH) and neutron stars (NS) by LIGO/Virgo have stimulated interest in the origin of the progenitor binaries. Dense stellar systems - globular and nuclear star clusters -
Autor:
Macintosh, B, Graham, JR, Barman, T, De Rosa, RJ, Konopacky, Q, Marley, MS, Marois, C, Nielsen, EL, Pueyo, L, Rajan, A, Rameau, J, Saumon, D, Wang, JJ, Patience, J, Ammons, M, Arriaga, P, Artigau, E, Beckwith, S, Brewster, J, Bruzzone, S, Bulger, J, Burningham, B, Burrows, AS, Chen, C, Chiang, E, Chilcote, JK, Dawson, RI, Dong, R, Doyon, R, Draper, ZH, Duchêne, G, Esposito, TM, Fabrycky, D, Fitzgerald, MP, Follette, KB, Fortney, JJ, Gerard, B, Goodsell, S, Greenbaum, AZ, Hibon, P, Hinkley, S, Cotton, TH, Hung, LW, Ingraham, P, Johnson-Groh, M, Kalas, P, Lafreniere, D, Larkin, JE, Lee, J, Line, M, Long, D, Maire, J, Marchis, F, Matthews, BC, Max, CE, Metchev, S, Millar-Blanchaer, MA, Mittal, T, Morley, CV, Morzinski, KM, Murray-Clay, R, Oppenheimer, R, Palmer, DW, Patel, R, Perrin, MD, Poyneer, LA, Rafikov, RR, Rantakyrö, FT, Rice, EL, Rojo, P, Rudy, AR, Ruffio, JB, Ruiz, MT, Sadakuni, N, Saddlemyer, L, Salama, M, Savransky, D, Schneider, AC, Sivaramakrishnan, A, Song, I, Soummer, R, Thomas, S, Vasisht, G
Publikováno v:
Macintosh, B; Graham, JR; Barman, T; De Rosa, RJ; Konopacky, Q; Marley, MS; et al.(2015). Discovery and spectroscopy of the young jovian planet 51 Eri b with the Gemini Planet Imager. Science, 350(6256), 64-67. doi: 10.1126/science.aac5891. UCLA: Retrieved from: http://www.escholarship.org/uc/item/5rg522fk
Directly detecting thermal emission from young extrasolar planets allows measurement of their atmospheric compositions and luminosities, which are influenced by their formation mechanisms. Using the Gemini Planet Imager, we discovered a planet orbiti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______325::410add22b0dad023b77946cf0623e63c
http://www.escholarship.org/uc/item/5rg522fk
http://www.escholarship.org/uc/item/5rg522fk
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