output
19912026
most citedObservation of a new particle in the search for the Standard Model Higgs boson with the ATLAS detector at the LHC

10.9k citations

Showing 2006 · astro-phShow all

23 papers · 2 filters

astro-ph2006★ 1.4k cited

Neutron Star Observations: Prognosis for Equation of State Constraints

James M. Lattimer, Maddapa Prakash

We investigate how current and proposed observations of neutron stars can lead to an understanding of the state of their interiors and the key unknowns: the typical neutron star ra…

astro-ph2006★ 55 cited

Detection of HNC and tentative detection of CN at z=3.9

M. Guelin, P. Salome, R. Neri +8

Molecular line emission from high-redshift galaxies holds great promise for the study of galaxy formation and evolution. The weak signals can only be detected with the largest mm-w…

astro-ph2006★ 46 cited

Propagation of the First Flames in Type Ia Supernovae

M. Zingale, L. J. Dursi

We consider the competition of the different physical processes that can affect the evolution of a flame bubble in a Type Ia supernovae -- burning, turbulence and buoyancy. Even in…

astro-ph2006★ 123 cited

Temporal Evolution of Coronagraphic Dynamic Range, and Constraints on Companions to Vega

Sasha Hinkley, Ben R. Oppenheimer, Remi Soummer +8

The major obstacle to the direct detection of companions to nearby stars is the overwhelming brightness of the host star. Current instruments employing the combination of adaptive…

astro-ph2006★ 53 cited

Dynamical Mass Estimates for Incomplete Orbits: Young Multiple Stars in Taurus and Ophiuchus

G. H. Schaefer, M. Simon, T. L. Beck +2

We present recent measurements of the orbital motion in the binaries, DF Tau and ZZ Tau, and in the triples, Elias 12, T Tau, and V853 Oph. We observed these systems with the Fine…

astro-ph2006★ 36 cited

Early spectral evolution of Nova Sgr 2004 (V5114 Sgr)

A. Ederoclite, E. Mason, M. Della Valle +15

We present optical and near-infrared spectral evolution of the Galactic nova V5114 Sgr (2004) during few months after the outburst. We use multi-band photometry and line intensitie…