Search Results - "Fabrycky, D"

Tidal dissipation in satellites prevents Hill sphere escape by Kisare, A M, Fabrycky, D C

“…ABSTRACT The transit method is a promising means of detecting exomoons, but few candidates have been identified. For planets close to their stars, the…”
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KEPLER-413B: A SLIGHTLY MISALIGNED, NEPTUNE-SIZE TRANSITING CIRCUMBINARY PLANET by Kostov, V B, McCullough, P R, Carter, J A, Deleuil, M, Diaz, R F, Fabrycky, D C, Hebrard, G, Hinse, T C, Mazeh, T, Orosz, J A, Tsvetanov, Z I, Welsh, W F

“…We report the discovery of a transiting, R sub(p) = 4.347 + or - 0.099R sub([+ in circle]), circumbinary planet (CBP) orbiting the Kepler K + M eclipsing…”
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ARE THE KEPLER NEAR-RESONANCE PLANET PAIRS DUE TO TIDAL DISSIPATION? by Lee, Man Hoi, Fabrycky, D, Lin, D N C

“…The multiple-planet systems discovered by the Kepler mission show an excess of planet pairs with period ratios just wide of exact commensurability for…”
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ROTATIONAL VELOCITIES OF INDIVIDUAL COMPONENTS IN VERY LOW MASS BINARIES by KONOPACKY, Q. M, GHEZ, A. M, FABRYCKY, D. C, MACINTOSH, B. A, WHITE, R. J, BARMAN, T. S, RICE, E. L, HALLINAN, G, DUCHENE, G

“…We present rotational velocities for individual components of 11 very low mass (VLM) binaries with spectral types between M7 and L7.5. These results are based…”
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Multiperiodic Galactic field RR Lyrae stars in the ASAS catalogue by Szczygieł, D. M., Fabrycky, D. C.

“…The All Sky Automated Survey (ASAS) monitors bright stars (8 < V < 14 mag) south of declination +28°. The ASAS Catalogue of Variable Stars (ACVS) presently…”
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The architecture of the hierarchical triple star KOI 928 from eclipse timing variations seen in Kepler photometry by Steffen, J. H., Quinn, S. N., Borucki, W. J., Brugamyer, E., Bryson, S. T., Buchhave, L. A., Cochran, W. D., Endl, M., Fabrycky, D. C., Ford, E. B., Holman, M. J., Jenkins, J., Koch, D., Latham, D. W., MacQueen, P., Mullally, F., Prša, A., Ragozzine, D., Rowe, J. F., Sanderfer, D. T., Seader, S. E., Short, D., Shporer, A., Thompson, S. E., Torres, G., Twicken, J. D., Welsh, W. F., Windmiller, G.

“…ABSTRACT We present a hierarchical triple star system (KIC 9140402) where a low‐mass eclipsing binary orbits a more massive third star. The orbital period of…”
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Starspots and spin-orbit alignment for Kepler cool host stars by Sanchis-Ojeda, R., Winn, J.N., Fabrycky, D.C.

“…The angle between the spin axis of the host star and the orbit of its planets (i.e., the stellar obliquity) is precious information about the formation and…”
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All-Sky Automated Survey eclipsing binaries with observed high period change rates by Pilecki, B., Fabrycky, D., Poleski, R.

“…We present 31 bright eclipsing contact and semidetached binaries that showed high period change rates (HPCRs) in a 5-yr interval in observations by the All-Sky…”
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Rapid multiperiodic variability in a Small Magellanic Cloud high-mass X-ray binary by Fabrycky, Daniel

“…The positions of high-mass X-ray binaries are often known precisely enough to identify the optical component unambiguously, and a number of those stars are or…”
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Shrinking Binary and Planetary Orbits by Kozai Cycles with Tidal Friction by Fabrycky, Daniel, Tremaine, Scott

“…At least two arguments suggest that the orbits of a large fraction of binary stars and extrasolar planets shrank by 1-2 orders of magnitude after formation:…”
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Planet Hunters IX. KIC 8462852 – where's the flux? by Boyajian, T. S., LaCourse, D. M., Rappaport, S. A., Fabrycky, D., Fischer, D. A., Gandolfi, D., Kennedy, G. M., Korhonen, H., Liu, M. C., Moor, A., Olah, K., Vida, K., Wyatt, M. C., Best, W. M. J., Brewer, J., Ciesla, F., Csák, B., Deeg, H. J., Dupuy, T. J., Handler, G., Heng, K., Howell, S. B., Ishikawa, S. T., Kovács, J., Kozakis, T., Kriskovics, L., Lehtinen, J., Lintott, C., Lynn, S., Nespral, D., Nikbakhsh, S., Schawinski, K., Schmitt, J. R., Smith, A. M., Szabo, Gy, Szabo, R., Viuho, J., Wang, J., Weiksnar, A., Bosch, M., Connors, J. L., Goodman, S., Green, G., Hoekstra, A. J., Jebson, T., Jek, K. J., Omohundro, M. R., Schwengeler, H. M., Szewczyk, A.

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Planet Hunters IX. KIC 8462852 – where's the flux? by Boyajian, T. S., LaCourse, D. M., Rappaport, S. A., Fabrycky, D., Fischer, D. A., Gandolfi, D., Kennedy, G. M., Korhonen, H., Liu, M. C., Moor, A., Olah, K., Vida, K., Wyatt, M. C., Best, W. M. J., Brewer, J., Ciesla, F., Csák, B., Deeg, H. J., Dupuy, T. J., Handler, G., Heng, K., Howell, S. B., Ishikawa, S. T., Kovács, J., Kozakis, T., Kriskovics, L., Lehtinen, J., Lintott, C., Lynn, S., Nespral, D., Nikbakhsh, S., Schawinski, K., Schmitt, J. R., Smith, A. M., Szabo, Gy, Szabo, R., Viuho, J., Wang, J., Weiksnar, A., Bosch, M., Connors, J. L., Goodman, S., Green, G., Hoekstra, A. J., Jebson, T., Jek, K. J., Omohundro, M. R., Schwengeler, H. M., Szewczyk, A.

“…Over the duration of the Kepler mission, KIC 8462852 was observed to undergo irregularly shaped, aperiodic dips in flux of up to ∼20 per cent. The dipping…”
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Kepler-36: A Pair of Planets with Neighboring Orbits and Dissimilar Densities by Carter, Joshua A., Agol, Eric, Chaplin, William J., Basu, Sarbani, Bedding, Timothy R., Buchhave, Lars A., Christensen-Dalsgaard, Jørgen, Deck, Katherine M., Elsworth, Yvonne, Fabrycky, Daniel C., Ford, Eric B., Fortney, Jonathan J., Hale, Steven J., Handberg, Rasmus, Hekker, Saskia, Holman, Matthew J., Huber, Daniel, Karoff, Christopher, Kawaler, Steven D., Kjeldsen, Hans, Lissauer, Jack J., Lopez, Eric D., Lund, Mikkel N., Lundkvist, Mia, Metcalfe, Travis S., Miglio, Andrea, Rogers, Leslie A., Stello, Dennis, Borucki, William J., Bryson, Steve, Christiansen, Jessie L., Cochran, William D., Geary, John C., Gilliland, Ronald L., Haas, Michael R., Hall, Jennifer, Howard, Andrew W., Jenkins, Jon M., Klaus, Todd, Koch, David G., Latham, David W., MacQueen, Phillip J., Sasselov, Dimitar, Steffen, Jason H., Twicken, Joseph D., Winn, Joshua N.

“…In the solar system, the planets' compositions vary with orbital distance, with rocky planets in close orbits and lower-density gas giants in wider orbits. The…”
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Radiative Thrusters on Close-in Extrasolar Planets by Fabrycky, Daniel

“…The atmospheres of close-in extrasolar planets absorb most of the incident stellar radiation, advert this energy, then reradlate photons in preferential…”
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Cassini States with Dissipation: Why Obliquity Tides Cannot Inflate Hot Jupiters by Fabrycky, Daniel C, Johnson, Eric T, Goodman, Jeremy

“…Some short-period exoplanets ("hot Jupiters") are observed by their transits to have anomalously large radii. It has been suggested that these planets are in a…”
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Catalog of Fundamental-Mode RR Lyrae Stars in the Galactic Bulge from the Optical Gravitational Lensing Experiment by Collinge, Matthew J, Sumi, Takahiro, Fabrycky, Daniel

“…We present a catalog of 1888 fundamental-mode RR Lyrae stars detected in the Galactic bulge fields of the second phase of the Optical Gravitational Lensing…”
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All-Sky Automated Survey eclipsing binaries with observed high period change rates by Pilecki, B., Fabrycky, D., Poleski, R.

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Multiperiodic Galactic field RR Lyrae stars in the ASAS catalogue by Szczygieł, D. M., Fabrycky, D. C.

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Planet Hunters IX. KIC 8462852 - where's the flux? by Boyajian, T S, LaCourse, D M, Rappaport, S A, Fabrycky, D, Fischer, D A, Gandolfi, D, Kennedy, G M, Korhonen, H, Liu, M C, Moor, A, Olah, K, Vida, K, Wyatt, M C, Best, W MJ, Brewer, J, Ciesla, F, Csak, B, Deeg, H J, Dupuy, T J, Handler, G, Heng, K, Howell, S B, Ishikawa, S T, Kovacs, J, Kozakis, T, Kriskovics, L, Lehtinen, J, Lintott, C, Lynn, S, Nespral, D, Nikbakhsh, S, Schawinski, K, Schmitt, J R, Smith, A M, Szabo, Gy, Szabo, R, Viuho, J, Wang, J, Weiksnar, A, Bosch, M, Connors, J L, Goodman, S, Green, G, Hoekstra, A J, Jebson, T, Jek, K J, Omohundro, M R, Schwengeler, H M, Szewczyk, A

“…Over the duration of the Kepler mission, KIC 8462852 was observed to undergo irregularly shaped, aperiodic dips in flux of up to ~20 per cent. The dipping…”
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Rotational Velocities of Individual Components in Very Low Mass Binaries by Konopacky, Q. M, Ghez, A. M, Fabrycky, D. C, Macintosh, B. A, White, R. J, Barman, T. S, Rice, E. L, Hallinan, G, Duchene, G

“…We present rotational velocities for individual components of eleven very low mass (VLM) binaries with spectral types between M7 and L7.5. These results are…”
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