output
19922026
most citedDirect Evidence for Neutrino Flavor Transformation from Neutral-Current Interactions in the Sudbury Neutrino Observatory

3k citations

Showing 2001 · astro-phShow all

10 papers · 2 filters

astro-ph2001★ 94 cited

(Sub)millimetre emission from NGC 1569: an abundance of very small grains

U. Lisenfeld, F. P. Isreal, J. M. Stil +1

We present new data of the dwarf galaxy NGC 1569 at 450 m, 850 m and 1200m taken with SCUBA at the JCMT and the bolometer array at the IRAM 30m telescope. After including…

astro-ph2001★ 127 cited

The formation of Uranus and Neptune among Jupiter and Saturn

Edward W. Thommes, Martin J. Duncan, Harold F. Levison

The outer giant planets, Uranus and Neptune, pose a challenge to theories of planet formation. They exist in a region of the Solar System where long dynamical timescales and a low…

astro-ph2001★ 25 cited

The `remarkable' M31 globular cluster 037-B327 revisited

Pauline Barmby, Kathryn M. Perrett, Terry J. Bridges

The M31 globular cluster candidate 037-B327 has long been known to be an extremely red, non-stellar object. The first published spectrum of this object is used to confirm that it i…

astro-ph2001★ 52 cited

NGC 5775: anatomy of a disk-halo interface

S. -W. Lee, J. A. Irwin, R. -J. Dettmar +3

We present the first high-resolution study of the disk-halo interface in an edge-on galaxy (NGC 5775) in which every component of the interstellar medium is represented and resolve…

astro-ph2001★ 10 cited

Protostellar Evolution during Time Dependent, Anisotropic Collapse

Mahmoud Aburihan, Jason D. Fiege, Richard N. Henriksen +1

The formation and collapse of a protostar involves the simultaneous infall and outflow of material in the presence of magnetic fields, self-gravity, and rotation. We use self-simil…

astro-ph2001★ 33 cited

GSH 138-01-94, an old supernova remnant in the far outer Galaxy

J. M. Stil, Judith A. Irwin

The properties of the Galactic HI shell GSH 138-01-94 are derived from data of the Canadian Galactic Plane Survey. The basic parameters of GSH 138-01-94 were determined by fitting…