output
20022026
most citedGeneralized Global Symmetries

1.7k citations

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17 papers · 1 filter

astro-ph2008★ 70 cited

Nearby young stars selected by proper motion. I. Four new members of the Beta Pictoris moving group from the Tycho-2 catalog

Sebastien Lepine, Michal Simon

We describe a procedure to identify stars from nearby moving groups and associations out of catalogs of stars with large proper motions. We show that from the mean motion vector of…

astro-ph2008★ 261 cited

The stellar association around Gamma Velorum and its relationship with Vela OB2

R. D Jeffries, Tim Naylor, F. M. Walter +2

We present the results of a photometric BVI survey of 0.9 square degrees around the Wolf-Rayet binary gamma^2 Vel and its early-type companion gamma^1 Vel. Several hundred PMS star…

astro-ph2008★ 37 cited

The Case for Hypercritical Accretion in M33 X-7

E. Moreno Mendez, G. E. Brown, C. -H. Lee +1

The spin parameter of the black hole in M33 X-7 has recently been measured to be a*=0.77+-0.05 (Liu et al. 2008). It has been proposed that the spin of the 15.65 M_sun black hole i…

astro-ph2008★ 15 cited

The Highly Eccentric Pre-Main Sequence Spectroscopic Binary RX J0529.3+1210

G. N. Mace, L. Prato, L. H. Wasserman +3

The young system RX J0529.3+1210 was initially identified as a single-lined spectroscopic binary. Using high-resolution infrared spectra, acquired with NIRSPEC on Keck II, we measu…

astro-ph2008★ 53 cited

The Star Formation Rate - Dense Gas Relation in Galaxies as Measured by HCN (3-2) Emission

R. S. Bussmann, D. Narayanan, Y. L. Shirley +6

We present observations made with the 10m Heinrich Hertz Sub-Millimeter Telescope of HCN (3-2) emission from a sample of 30 nearby galaxies ranging in infrared luminosity from 10^1…

astro-ph2008★ 7 cited

Variability in the cycle length of the supersoft source RX J0513.9-6951

V. Burwitz, K. Reinsch, J. Greiner +4

The supersoft X-ray binary RX J0513.9-6951 shows cyclic changes between optical-low / X-ray-on states and optical-high / X-ray-off states. It is supposed to be accreting close to t…