output
20022009
most citedWeak magnetic fields in Ap/Bp stars: Evidence for a dipole field lower limit and a tentative interpretation of the magnetic dichotomy

296 citations

Showing 2006 · astro-phShow all

19 papers · 2 filters

astro-ph200666 cited

ACS photometry of newly-discovered globular clusters in the outer halo of M31

A. D. Mackey, A. Huxor, A. M. N. Ferguson +6

We report the first results from deep ACS imaging of ten classical globular clusters in the far outer regions (15 < R_p < 100 kpc) of M31. Eight of the clusters, including two of t…

astro-ph200626 cited

Rotation and chemical abundances of Ap/Bp stars in the open cluster NGC 6475

C. P. Folsom, G. A. Wade, S. Bagnulo +1

The connection between age, rotation and chemical abundance of magnetic Ap stars is poorly understood. Using open clusters, we are able to study samples of stars that are both co-e…

astro-ph200693 cited

ACS photometry of extended, luminous globular clusters in the outskirts of M31

A. D. Mackey, A. Huxor, A. M. N. Ferguson +6

A new population of extended, luminous globular clusters has recently been discovered in the outskirts of M31. These objects have luminosities typical of classical globular cluster…

astro-ph2006

The Possible Belts for Extrasolar Planetary Systems

Ing-Guey Jiang, M. Duncan, D. N. C. Lin

More than 100 extrasolar planets have been discovered since 1990s. Different from the solar system, these planets' orbital eccentricities cover a huge range from 0 to 0.7. Incident…

astro-ph200643 cited

A Deep Wide-Field Variable Star Catalog of Omega Centauri

David T. F Weldrake, Penny D Sackett, Terry J Bridges

We present a variable star catalog of an extensive ground-based wide-field variability survey in the globular cluster omega Centauri. Using the ANU 40-inch (1m) telescope at Siding…

astro-ph200634 cited

The Faint End of the Luminosity Function in the Core of the Coma Cluster

M. L. Milne, C. J. Pritchet, G. B. Poole +4

We present optical measurements of the faint end of the luminosity function in the core of the Coma cluster. Dwarf galaxies are detected down to a limiting magnitude of R approx. 2…