Last 7 days     Results 2421-2440 of 27323.   117 118 119 120 121 122 123 124 125 126 127   WASP-20b and WASP-28b: a hot Saturn and a hot Jupiter in near-aligned orbits around solar-type starsAnderson, D. R.; Collier Cameron, A.; Hellier, C. et alE-print/Working paper (2014)We report the discovery of the planets WASP-20b and WASP-28b along with measurements of their sky-projected orbital obliquities. WASP-20b is an inflated, Saturn-mass planet (0.31 $M_{\rm Jup}$; 1.46 $R ... [more ▼]We report the discovery of the planets WASP-20b and WASP-28b along with measurements of their sky-projected orbital obliquities. WASP-20b is an inflated, Saturn-mass planet (0.31$M_{\rm Jup}$; 1.46$R_{\rm Jup}) in a 4.9-day, near-aligned (\lambda = 8.1 \pm 3.6^\circ$) orbit around CD-24 102 ($V$=10.7; F9). WASP-28b is an inflated, Jupiter-mass planet (0.91$M_{\rm Jup}$; 1.21$R_{\rm Jup}) in a 3.4-day, near-aligned (\lambda = 8 \pm 18^\circ$) orbit around a$V$=12, F8 star. As intermediate-mass planets in short orbits around aged, cool stars ($7^{+2}_{-1}$Gyr for WASP-20 and$5^{+3}_{-2}$Gyr for WASP-28; both with$T_{\rm eff}\$ < 6250 K), their orbital alignment is consistent with the hypothesis that close-in giant planets are scattered into eccentric orbits with random alignments, which are then circularised and aligned with their stars' spins via tidal dissipation. [less ▲]Detailed reference viewed: 12 (0 ULg) Alignment in star-debris disc systems seen by HerschelGreaves, J. S.; Kennedy, G. M.; Thureau, N. et alin Monthly Notices of the Royal Astronomical Society : Letters (2014), 438Many nearby main-sequence stars have been searched for debris using the far-infrared Herschel satellite, within the DEBRIS, DUNES and Guaranteed-Time Key Projects. We discuss here 11 stars of spectral ... [more ▼]Many nearby main-sequence stars have been searched for debris using the far-infrared Herschel satellite, within the DEBRIS, DUNES and Guaranteed-Time Key Projects. We discuss here 11 stars of spectral types A-M where the stellar inclination is known and can be compared to that of the spatially resolved dust belts. The discs are found to be well aligned with the stellar equators, as in the case of the Sun's Kuiper belt, and unlike many close-in planets seen in transit surveys. The ensemble of stars here can be fitted with a star-disc tilt of ≲ 10°. These results suggest that proposed mechanisms for tilting the star or disc in fact operate rarely. A few systems also host imaged planets, whose orbits at tens of au are aligned with the debris discs, contrary to what might be expected in models where external perturbers induce tilts. [less ▲]Detailed reference viewed: 11 (0 ULg) Archéologies de l'abstraction. Sur quelques récentes en philosophie des sciencesCavazzini, Andrea Scientific conference (2014, February 01)Detailed reference viewed: 10 (0 ULg) CoMBiSpeC: A novel approach in the modelling of massive binariesPalate, Matthieu in EAS Publications Series (2014, February 01)Spectral modelling and especially for massive stars is not a straightforward problem and over the past decades many advances have been made in this field. We now have sophisticated model atmosphere codes ... [more ▼]Spectral modelling and especially for massive stars is not a straightforward problem and over the past decades many advances have been made in this field. We now have sophisticated model atmosphere codes that allow to derive the stellar parameters. However, these codes are based on the assumption that the star is single and spherical which is no longer valid for the components of a binary system. On the other hand, observational studies indicate that binarity has an impact on the spectra. This is why we have developed a model called CoMBiSpeC (code of massive binary spectral computation) that specifically accounts for the impact of binarity on the spectra. [less ▲]Detailed reference viewed: 8 (1 ULg) Où en est la recherche sur les dysphasies ?Maillart, Christelle Conference given outside the academic context (2014)Detailed reference viewed: 67 (2 ULg) A multi-method approach to radial-velocity measurement for single-object spectraDavid, M.; Blomme, R.; Frémat, Y. et alin Astronomy and Astrophysics (2014), 562Context. The derivation of radial velocities from large numbers of spectra that typically result from survey work, requires automation. However, except for the classical cases of slowly rotating late-type ... [more ▼]Context. The derivation of radial velocities from large numbers of spectra that typically result from survey work, requires automation. However, except for the classical cases of slowly rotating late-type spectra, existing methods of measuring Doppler shifts require fine-tuning to avoid a loss of accuracy due to the idiosyncrasies of individual spectra. The radial velocity spectrometer (RVS) on the Gaia mission, which will start operating very soon, prompted a new attempt at creating a measurement pipeline to handle a wide variety of spectral types.