output
20062025
most citedMass loss from hot massive stars

644 citations

researchers with a paper here

Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.

collaborating institutions
Showing 2008 · astro-phShow all

5 papers · 2 filters

astro-ph2008★ 96 cited

Physical properties of galaxies and their evolution in the VIMOS VLT Deep Survey. I. The evolution of the mass-metallicity relation up to z~0.9

F. Lamareille, J. Brinchmann, T. Contini +43

We derive the mass-metallicity relation of star-forming galaxies up to , using data from the VIMOS VLT Deep Survey. Automatic measurement of emission-line fluxes and equi…

astro-ph2008★ 644 cited

Mass loss from hot massive stars

J. Puls, J. S. Vink, F. Najarro

Mass loss is a key process in the evolution of massive stars, and must be understood quantitatively to be successfully included in broader astrophysical applications. In this revie…

astro-ph2008★ 41 cited

HVS7: a chemically peculiar hyper-velocity star

N. Przybilla, M. F. Nieva, A. Tillich +3

Context: Hyper-velocity stars are suggested to originate from the dynamical interaction of binary stars with the supermassive black hole in the Galactic centre (GC), which accelera…

astro-ph2008★ 76 cited

The supermassive black hole of Fornax A

N. Nowak, R. P. Saglia, J. Thomas +3

The radio galaxy Fornax A (NGC 1316) is a prominent merger remnant in the outskirts of the Fornax cluster. Its giant radio lobes suggest the presence of a powerful AGN and thus a c…

astro-ph2008★ 62 cited

LMC origin of the hyper-velocity star HE 0437-5439. Beyond the supermassive black hole paradigm

N. Przybilla, M. F. Nieva, U. Heber +4

Context: Hyper-velocity stars move so fast that only a supermassive black hole (SMBH) seems to be capable to accelerate them. Hence the Galactic centre (GC) is their only suggested…