activity
19992008
most citedArgon Abundances in the Solar Neighborhood: Non-LTE Analysis of Orion Association B-type Stars

40 citations · 40 across the 4 of their papers we have counts for

collaborators

7 papers

astro-ph2008

The Gaia satellite: a tool for Emission Line Stars and Hot Stars

Christophe Martayan, Yves Fremat, Ronny Blomme +19

The Gaia satellite will be launched at the end of 2011. It will observe at least 1 billion stars, and among them several million emission line stars and hot stars. Gaia will provid…

astro-ph200740 cited

Argon Abundances in the Solar Neighborhood: Non-LTE Analysis of Orion Association B-type Stars

Thierry Lanz, Katia Cunha, Jon Holtzman +1

Argon abundances have been derived for a sample of B main-sequence stars in the Orion association. The abundance calculations are based on NLTE metal line-blanketed model atmospher…

astro-ph2007

A Mid-Infrared Spitzer Study of the Herbig Be Star R Mon and the Associated HH 39 Herbig-Haro Object

M. Audard, S. Skinner, M. Guedel +3

We report on initial results of our Spitzer Cycle 2 program to observe the young massive star R Mon and its associated HH 39 Herbig-Haro object in the mid-infrared. Our program use…

astro-ph2006

Modeling multidimensional effects in the propagation of radiative shocks

Sébastien Leygnac, Laurent Boireau, Claire Michaut +4

Radiative shocks (also called supercritical shocks) are high Mach number shock waves that photoionize the medium ahead of the shock front and give rise to a radiative precursor. Th…

astro-ph2006

A Grid of NLTE Line-Blanketed Model Atmospheres of Early B-type Stars

Thierry Lanz, Ivan Hubeny

We have constructed a comprehensive grid of 1540 metal line-blanketed, NLTE, plane-parallel, hydrostatic model atmospheres for the basic parameters appropriate to early B-type star…

astro-ph2002

A New Formation Mechanism for the Hottest Horizontal-Branch Stars

Allen V. Sweigart, Thomas M. Brown, Thierry Lanz +2

Stars with very large mass loss on the red-giant branch can undergo the helium flash while descending the white-dwarf cooling curve. Under these conditions the flash convection zon…