4.7 Article

THE CONNECTION BETWEEN A LYMAN LIMIT SYSTEM, A VERY STRONG O VI ABSORBER, AND GALAXIES AT z ∼ 0.203

Related references

Note: Only part of the references are listed.
Article Astronomy & Astrophysics

On the HI content, dust-to-gas ratio and nature of MgII absorbers

Brice Menard et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2009)

Review Astronomy & Astrophysics

Mass, metal, and energy feedback in cosmological simulations

Benjamin D. Oppenheimer et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2008)

Article Astronomy & Astrophysics

Towards understanding the mass-metallicity relation of quasar absorbers:: evidence for bimodality and consequences

Nicolas Bouche

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2008)

Article Astronomy & Astrophysics

The recycling of gas and metals in galaxy formation: predictions of a dynamical feedback model

Serena Bertone et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2007)

Article Astronomy & Astrophysics

A large population of metal-rich, compact, intergalactic CIV absorbers - evidence for poor small-scale metal mixing

Joop Schaye et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2007)

Article Astronomy & Astrophysics

Highly ionized plasma in the Large Magellanic Cloud: evidence for outflows and a possible galactic wind

N. Lehner et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2007)

Article Astronomy & Astrophysics

CalFUSE version 3:: A data reduction pipeline for the Far Ultraviolet Spectroscopic Explorer

W. V. Dixon et al.

PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC (2007)

Article Astronomy & Astrophysics

A new look at the large-scale HI structure of the Large Magellanic Cloud

L Staveley-Smith et al.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2003)