activity
19972011
most citedDense Matter in Compact Stars: Theoretical Developments and Observational Constraints

218 citations · 778 across the 46 of their papers we have counts for

collaborators

90 papers

astro-ph.GA20099 cited

Diffuse continuum transfer in H II regions

R. J. R. Williams, W. J. Henney

We compare the accuracy of various methods for determining the transfer of the diffuse Lyman continuum in HII regions, by comparing them with a high-resolution discrete-ordinate in…

hep-ph20097 cited

Decays Z --> ggg and Z-prime --> ggg in the minimal 331 model

A. Flores-Tlalpa, J. Montano, F. Ramirez-Zavaleta +1

We perform a complete calculation at the one-loop level for the Zggg and Z'ggg couplings in the context of the minimal 331 model, which predicts the existence of a new Z' gauge bos…

astro-ph.CO2009

Age and Extinction of the Ultraviolet Emitting Regions in M82

L. H. Rodriguez-Merino, D. Rosa-Gonzalez, Y. D. Mayya +3

The M82 galaxy has been the subject of several studies basically because it is relatively close to to the Milky Way and it displays a strong star formation activity. Using multi-ba…

astro-ph.CO20091 cited

M82 as a Galaxy: Morphology and Stellar Content of the Disk and Halo

Y. Divakara Mayya, Luis Carrasco

For decades, the nuclear starburst has taken all the limelight in M82 with very little discussion on M82 as a galaxy. The situation is changing over the last decade, with the publi…

astro-ph.GA2009

The energetic environment and the dense interstellar medium in ULIRGs

O. Vega, M. S. Clemens, A. Bressan +3

We fit the near-infrared to radio spectral energy distributions of a sample of 30 luminous and ultra-luminous infrared galaxies with models that include both starburst and AGN comp…

astro-ph200812 cited

A likely optical counterpart of the G292.0+1.8 pulsar wind nebula

S. V. Zharikov, Yu. A. Shibanov, D. A. Zyuzin +2

G292.0+1.8 is the Cas A-like supernova remnant containing the young pulsar PSR J1124-5916, which powers a compact torus-like pulsar wind nebula with a jet visible in X-rays. We hav…