Zobrazeno 1 - 10
of 734
pro vyhledávání: '"M J, Holman"'
Autor:
J. Kleyna, Ignacio Ferrin, William T. Reach, James M. Bauer, Veronica Motta, J. Pittichová, Yanga R. Fernandez, David J. Osip, Steven R. Chesley, Tetsuharu Fuse, Karen J. Meech, M. J. Holman, Carey M. Lisse, Olivier Hainaut, P. Challis, Stephen C. Lowry, Eric Christensen, T. Brink, M. F. A'Hearn, Donald K. Yeomans, M. Mateo, Amy Mainzer
Publikováno v:
Icarus. 222:662-678
Comet 85P/Boethin was selected as the original comet target for the Deep Impact extended mission, EPOXI . Because this comet had been only observed at two apparitions in 1975 and 1986 and consequently had a large ephemeris error, an early intense rec
Autor:
M. J. Holman
Publikováno v:
EAS Publications Series. 42:39-54
Surveys for transiting extrasolar planets, including the space-based missions CoRoT and Kepler, are expected to detect hundreds of Jovian mass planets and tens of terrestrial mass planets. For many of these newly discovered planets, the intervals bet
Autor:
Penny D. Sackett, Dimitar Sasselov, M. J. Holman, Cristina Afonso, Robert W. Noyes, András Pál, Andrés Jordán, Gábor L. Kovács, Gáspár Á. Bakos, Th. Henning, Z. Csubry
Publikováno v:
Proceedings of the International Astronomical Union. 4:354-357
HAT-South is a network of six identical, fully automated wide field telescopes, to be located at three sites (Chile: Las Campanas, Australia: Siding Springs, and Namibia: HESS site) in the Southern hemisphere. The primary purpose of the network is to
Publikováno v:
Graft. 5:344-351
Publikováno v:
The Astrophysical Journal. 565:608-620
We examine the eccentricity evolution of a system of two planets locked in a mean motion resonance, in which the outer planet loses energy and angular momentum. The sink of energy and angular momentum could be either a gas or planetesimal disk. We sh
Autor:
Alice C. Quillen, M. J. Holman
Publikováno v:
The Astronomical Journal. 119:397-402
During the orbital migration of a giant extrasolar planet via ejection of planetesimals (as studied by Murray et al. in 1998), inner mean-motion resonances can be strong enough to cause planetesimals to graze or impact the star. We integrate numerica
Publikováno v:
The Astronomical Journal. 116:2583-2589
We consider the effect of gravitational perturbations from Jupiter on the dynamics of asteroids, when Jupiter is itself perturbed by Saturn. The presence of Saturn introduces a number of additional frequencies into Jupiters orbit. These frequencies i
Publikováno v:
Infectious Disease Modelling (2468-2152). Sep2024, Vol. 9 Issue 3, p713-727. 15p.
Autor:
Søren Meibom, Jasonjot S. Kalirai, Joseph Barranco, B. S. Gaudi, Marc H. Pinsonneault, Brian A. McLeod, Joel D. Hartman, K. Z. Stanek, M. J. Holman
We present the results of a deep (15 ~< r ~< 23), 20 night survey for transiting planets in the intermediate age open cluster M37 (NGC 2099) using the Megacam wide-field mosaic CCD camera on the 6.5m MMT. We do not detect any transiting planets among
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::35e600e88d79585a490c3111e06653c1
Autor:
K. Z. Stanek, P. M. Garnavich, P. A. Nutzman, J. D. Hartman, A. Garg, K. Adelberger, P. Berlind, A. Z. Bonanos, M. L. Calkins, P. Challis, B. S. Gaudi, M. J. Holman, R. P. Kirshner, B. A. McLeod, D. Osip, T. Pimenova, T. H. Reiprich, W. Romanishin, T. Spahr, S. C. Tegler, X. Zhao
We present deep optical photometry of the afterglow of gamma-ray burst (GRB) 041006 and its associated hypernova obtained over 65 days after detection (55 R-band epochs on 10 different nights). Our early data (t
ApJ Letters, accepted. Additional
ApJ Letters, accepted. Additional
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::97a80db2ef894ec530b44f1b8941d95b
http://arxiv.org/abs/astro-ph/0502319
http://arxiv.org/abs/astro-ph/0502319