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20022026
most citedToward the Standard Population Synthesis Model of the X-Ray Background: Evolution of X-Ray Luminosity and Absorption Functions of Active Galactic Nuclei Including Compton-Thick Populations

676 citations

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6 papers · 1 filter

astro-ph2008★ 43 cited

Multiple and Precessing Collimated Outflows in the Planetary Nebula IC 4634

M. A. Guerrero, L. F. Miranda, A. Riera +6

With its remarkable double-S shape, IC 4634 is an archetype of point-symmetric planetary nebulae (PN). In this paper, we present a detailed study of this PN using archival HST WFPC…

astro-ph2008★ 5 cited

A First Estimate Of The X-Ray Binary Frequency As A Function Of Star Cluster Mass In A Single Galactic System

D. M. Clark, S. S. Eikenberry, B. R. Brandl +7

We use the previously-identified 15 infrared star-cluster counterparts to X-ray point sources in the interacting galaxies NGC 4038/4039 (the Antennae) to study the relationship bet…

astro-ph2008★ 17 cited

BF Eridani: a cataclysmic variable with a massive white dwarf and an evolved secondary

V. V. Neustroev, S. Zharikov

We present high- and medium-resolution spectroscopic observations of the cataclysmic variable BF Eri during its low and bright states. The orbital period of this system was found t…

astro-ph2007★ 35 cited

Large Scale Flows from Orion-South

W. J. Henney, C. R. O'Dell, Luis A. Zapata +3

Multiple optical outflows are known to exist in the vicinity of the active star formation region called Orion-South (Orion-S). We have mapped the velocity of low ionization feature…

astro-ph2003★ 2 cited

Relation between source and temperature fluctuations in photoionized nebulae

Luc Binette, Pierre Ferruit, Wolfgang Steffen +1

The magnitude of the temperature fluctuations (t^2) required to explain the observed inconsistencies between metallicities inferred from recombination lines and from forbidden line…

astro-ph2002★ 3 cited

N-Body Simulations of Small Galaxy Groups

Hector Aceves, Hector Velazquez

A series of N-body simulations aimed to study the dynamics of small groups of galaxies are presented. The properties of small galaxy groups are very well reproduced, and those of H…