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The recent Gaia Data Release 3 has unveiled a catalog of over eight hundred thousand binary systems, providing orbital solutions for half of them. Since most of them are unresolved astrometric binaries, several astrophysical parameters that…

太阳与恒星天体物理 · 物理学 2023-07-10 Xabier Pérez-Couto , Jose Á. Docobo , Pedro P. Campo

Gamma -ray bursts (GRBs) observed up to redshifts $z>9.4$ can be used as possible probes to test cosmological models. Here we show how changes of the slope of the {\it luminosity $L^*_X$ -break time $T^*_a$} correlation in GRB afterglows,…

高能天体物理现象 · 物理学 2015-06-16 Maria Giovanna Dainotti , Vincenzo Fabrizio Cardone , Ester Piedipalumbo , Salvatore Capozziello

The light curves of old G-dwarfs obtained in the visible and near-infrared wavelength ranges are highly irregular. This significantly complicates the detectability of the rotation periods of stars similar to the Sun in large photometric…

太阳与恒星天体物理 · 物理学 2025-02-26 Valeriy Vasilyev , Timo Reinhold , Alexander I. Shapiro , Theodosios Chatzistergos , Natalie Krivova , Sami K. Solanki

Solar gravity modes are considered as the {\it Rosetta Stone} for probing and subsequently deciphering the physical properties of the solar inner-most layers. Recent claims of positive detection therefore shed some new light on the…

太阳与恒星天体物理 · 物理学 2022-11-30 Kévin Belkacem , Charly Pinçon , Gaël Buldgen

We apply Monte Carlo projection to the radial velocity data set that Anglada Escude et al. (2016) use for the discovery of Proxima b. They find an upper limit to the orbital eccentricity of 0.35. To investigate the eccentricity issue…

地球与行星天体物理 · 物理学 2017-08-02 Robert A. Brown

We present new radial velocity measurements of the ultra-cool dwarf VB 10, which was recently announced to host a giant planet detected with astrometry. The new observations were obtained using optical spectrographs(MIKE/Magellan and…

地球与行星天体物理 · 物理学 2015-05-14 Guillem Anglada-Escude , Evgenya L. Shkolnik , Alycia J. Weinberger , Ian B. Thompson , David J. Osip , John H. Debes

We have observed 4 transits of the planet of HD 209458 using the STIS spectrograph on HST. Summing the recorded counts over wavelength between 582 nm and 638 nm yields a photometric time series with 80 s time sampling and relative precision…

天体物理学 · 物理学 2008-11-26 Timothy M. Brown , David Charbonneau , Ronald L. Gilliland , Robert W. Noyes , Adam Burrows

In the last years, a new generation of interplanetary space missions have been designed for the exploration of the solar system. At the same time, radio-science instrumentation has reached an unprecedented level of accuracy, leading to a…

地球与行星天体物理 · 物理学 2022-01-05 Giacomo Lari , Giulia Schettino , Daniele Serra , Giacomo Tommei

Gravity modes are the best probes to study the solar radiative zone dynamics, especially in the nuclear core. These modes remain difficult to observe, but they are essential ingredients for progressing on the evolution of the Sun-Earth…

天体物理学 · 物理学 2009-11-11 Sylvaine Turck-Chieze

The 3:2 spin-orbit resonance between the rotational and orbital motions of Mercury results from a functional dependance on a tidal friction adding to a non-zero eccentricity with a permanent asymmetry in the equatorial plane of the planet.…

天体物理学 · 物理学 2007-05-23 Nicolas Rambaux , Eric Bois

The standard cosmological model is assumed to respect parity symmetry. Under this assumption the cross-correlations of the CMB's temperature anisotropy and `gradient'-like polarization, with the `curl'-like polarization identically vanish…

宇宙学与河外天体物理 · 物理学 2009-10-29 N. J. Miller , M. Shimon , B. G. Keating

The mutual orbital alignment in multiple planetary systems is an important parameter for understanding their formation. There are a number of elaborate techniques to determine the alignment parameters using photometric or spectroscopic…

地球与行星天体物理 · 物理学 2021-12-29 Holger M. Müller , Panagiotis Ioannidis , Jürgen H. M. M. Schmitt

We search for new variable B-type pulsators in the CoRoT data assembled primarily for planet detection, as part of CoRoT's Additional Programme. We aim to explore the properties of newly discovered B-type pulsators from the uninterrupted…

The CMB's B-mode polarization provides a handle on several cosmological parameters most notably the tensor-to-scalar ratio, $r$, and is sensitive to parameters which govern the growth of large scale structure (LSS) and evolution of the…

天体物理学 · 物理学 2009-03-20 N. J. Miller , M. Shimon , B. G. Keating

The space missions MOST, COROT and Kepler are going to provide us with high-precision optical photometry of solar-like stars with time series extending from tens of days to several years. They can be modelled to obtain information on…

天体物理学 · 物理学 2008-11-26 A. F. Lanza , A. S. Bonomo , M. Rodono'

Planetary systems orbiting close binaries are valuable testing grounds for planet formation and migration models. More detections with good mass measurements are needed. We present a new planet discovered during the BEBOP survey for…

We argue that, in general, observational studies of Be-star rotation have paid insufficient attention to the effects of equatorial gravity darkening. We present new line-profile calculations that emphasize the insensitivity of line width to…

天体物理学 · 物理学 2011-05-12 Richard H. D. Townsend , Stanley P. Owocki , Ian D. Howarth

We perform a wavelet analysis of the temperature and polarization maps of the Cosmic Microwave Background (CMB) delivered by the WMAP experiment in search for a parity violating signal. Such a signal could be seeded by new physics beyond…

天体物理学 · 物理学 2008-11-26 Paolo Cabella , Paolo Natoli , Joseph Silk

The discovery of leptonic CP violation is one of the primary goals of next-generation neutrino oscillation experiments, which is feasible due to the recent measurement of a relatively large leptonic mixing angle \theta_{13}. We suggest two…

高能物理 - 唯象学 · 物理学 2013-03-19 Tommy Ohlsson , He Zhang , Shun Zhou

Signatures of coupling between an inertial mode in the convective core and a gravito-inertial mode in the envelope have been found in four-year Kepler light curves of 16 rapidly rotating $\gamma\,$Doradus ($\gamma\,$Dor) stars. This makes…

太阳与恒星天体物理 · 物理学 2023-09-06 Conny Aerts , Stéphane Mathis