Zobrazeno 1 - 8
of 8
pro vyhledávání: '"Tobias W. A. Müller"'
Publikováno v:
Proceedings of the VLDB Endowment. 11:1536-1549
SQL declaratively specifies what the desired output of a query is. This work shows that a non-standard interpretation of the SQL semantics can, instead, disclose where a piece of the output originated in the input and why that piece found its way int
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ba18471c771666bb8106ed4ac2226376
https://doi.org/10.14778/3236187.3236204
https://doi.org/10.14778/3236187.3236204
Autor:
Guillermo Torres, Eric Agol, Daniel Jontof-Hutter, Eric B. Ford, William F. Welsh, Michael Endl, Nader Haghighipour, Gur Windmiller, Billy Quarles, Sean M. Mills, Tobias W. A. Müller, Daniel C. Fabrycky, Tobias C. Hinse, William D. Cochran, Jack J. Lissauer, Donald R. Short, Jerome A. Orosz, Suman Satyal, Tsevi Mazeh
Of the nine confirmed transiting circumbinary planet systems, only Kepler-47 is known to contain more than one planet. Kepler-47 b (the "inner planet") has an orbital period of 49.5 days and a radius of about $3\,R_{\oplus}$. Kepler-47 c (the "outer
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::78da661dcd6687b9d3cda922857796e6
Autor:
William F. Welsh, Jerome A. Orosz, Donald R. Short, William D. Cochran, Michael Endl, Erik Brugamyer, Nader Haghighipour, Lars A. Buchhave, Laurance R. Doyle, Daniel C. Fabrycky, Tobias Cornelius Hinse, Stephen R. Kane, Veselin Kostov, Tsevi Mazeh, Sean M. Mills, Tobias W. A. Müller, Billy Quarles, Samuel N. Quinn, Darin Ragozzine, Avi Shporer, Jason H. Steffen, Lev Tal-Or, Guillermo Torres, Gur Windmiller, William J. Borucki
We present the discovery of KIC 9632895b, a 6.2 Earth-radius planet in a low-eccentricity, 240.5-day orbit about an eclipsing binary. The binary itself consists of a 0.93 and 0.194 solar mass pair of stars with an orbital period of 27.3 days. The pla
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d17c068ab62ac6bef17b0ae4d3e98da0
https://resolver.caltech.edu/CaltechAUTHORS:20151020-112216543
https://resolver.caltech.edu/CaltechAUTHORS:20151020-112216543
Autor:
Nader Haghighipour, Eric B. Ford, Daniel C. Fabrycky, Jack J. Lissauer, Guillermo Torres, Veselin B. Kostov, David W. Latham, Ilya Kull, Joshua Pepper, Eric L. N. Jensen, William F. Welsh, Jason H. Steffen, Geoffrey W. Marcy, Billy Quarles, Gur Windmiller, Tobias C. Hinse, Samuel N. Quinn, Donald R. Short, Joao Gregorio, Jon M. Jenkins, Tsevi Mazeh, Laurance R. Doyle, Tobias W. A. Müller, Darin Ragozzine, Stephen R. Kane, William J. Borucki, Michael Endl, Howard Isaacson, Avi Shporer, Jerome A. Orosz, William D. Cochran
We report the discovery of a new Kepler transiting circumbinary planet (CBP). This latest addition to the still-small family of CBPs defies the current trend of known short-period planets orbiting near the stability limit of binary stars. Unlike the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a6f5e063a4dbb6452b4026918b936cdf
Publikováno v:
The Astrophysical Journal. 782:26
We have developed a comprehensive methodology and an interactive Web site for calculating the habitable zone (HZ) of multiple star systems. Using the concept of spectral weight factor, as introduced in our previous studies of the calculations of HZ i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4b85615def1875312b2c30031d83fd62
https://doi.org/10.1088/0004-637x/782/1/26
https://doi.org/10.1088/0004-637x/782/1/26
Autor:
Tobias W. A. Müller, Wilhelm Kley
Publikováno v:
Astronomy & Astrophysics. 560:A40
Transitional disks are protoplanetary disk around young stars that display inner holes in the dust distribution within a few AU, which is accompanied nevertheless by some gas accretion onto the central star. These cavities could possibly be created b
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8ca0522e31dd00c8d6c71e901925ea45
https://doi.org/10.1051/0004-6361/201322503
https://doi.org/10.1051/0004-6361/201322503
Publikováno v:
Astronomy & Astrophysics. 541:A123
In 2D simulations of thin gaseous disks with embedded planets or self-gravity the gravitational potential needs to be smoothed to avoid singularities in the numerical evaluation of the gravitational potential or force. In order to correctly resemble
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9a6a451cd2423d8ee4276b2d16a1f6d5
https://doi.org/10.1051/0004-6361/201118737
https://doi.org/10.1051/0004-6361/201118737
Autor:
Jerome A. Orosz, William F. Welsh, Nader Haghighipour, Billy Quarles, Donald R. Short, Sean M. Mills, Suman Satyal, Guillermo Torres, Eric Agol, Daniel C. Fabrycky, Daniel Jontof-Hutter, Gur Windmiller, Tobias W. A. Müller, Tobias C. Hinse, William D. Cochran, Michael Endl, Eric B. Ford, Tsevi Mazeh, Jack J. Lissauer
Publikováno v:
Astronomical Journal; May2019, Vol. 157 Issue 5, p1-1, 1p