output
20042011
most citedSpectra and Light Curves of Six Type Ia Supernovae at 0.511 < z < 1.12 and the Union2 Compilation

1.4k citations

Showing astro-ph.SRShow all

8 papers · 1 filter

astro-ph.SR2011

EVLA observations of the nebula around G79.29+0.46

G. Umana, C. S. Buemi, C. Trigilio +5

We have observed the radio nebula surrounding the Galactic LBV candidate G79.29+0.46 with the EVLA at 6 cm. These new radio observations allow a morphological comparison between th…

astro-ph.SR201183 cited

X-ray illumination of the ejecta of Supernova 1987A

J. Larsson, C. Fransson, G. Östlin +25

We present the late-time optical light curve of the ejecta of SN 1987A measured from HST imaging observations spanning the past 17 years. We find that the flux from the ejecta decl…

astro-ph.SR2010163 cited

A precise asteroseismic age and radius for the evolved Sun-like star KIC 11026764

T. S. Metcalfe, M. J. P. F. G. Monteiro, M. J. Thompson +55

The primary science goal of the Kepler Mission is to provide a census of exoplanets in the solar neighborhood, including the identification and characterization of habitable Earth-…

astro-ph.SR201015 cited

VISIR/VLT and VLA joint imaging analysis of the circumstellar nebula around IRAS~18576+0341

C. S. Buemi, G. Umana, C. Trigilio +2

High spatial and sensitivity images of the Luminous Blue Variable IRAS 18576+0341 were obtained using the mid infrared imager VISIR at the Very Large Telescope and the Very Large A…

astro-ph.SR201035 cited

Photospheric activity, rotation, and star-planet interaction of the planet-hosting star CoRoT-6

A. F. Lanza, A. S. Bonomo, I. Pagano +13

The CoRoT satellite has recently discovered a hot Jupiter that transits across the disc of a F9V star called CoRoT-6 with a period of 8.886 days. We model the photospheric activity…

astro-ph.SR201032 cited

Characterization of Kepler early-type targets

G. Catanzaro, A. Frasca, J. Molenda-Zakowicz +1

Stellar pulsation offers a unique opportunity to constrain the intrinsic parameters of stars and unveil their inner structure. The Kepler satellite is collecting an enormous amount…