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The X - Ray Photoionized Wind in Cen X - 3 / V 779 Cen

We analyze the ASCA spectrum of the Cen X-3 X-ray binary system in eclipse using atomic models appropriate to recombination-dominated level population kinetics in an overionized plasma. In order to estimate the wind characteristics, we first fit the eclipse spectrum to a single-zone photoionized plasma model. We then fit spectra from a range of orbital phases using global models of photoionized...

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The acoustic spectrum of α Cen A ⋆

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The Variable Quiescence of Cen X - 4

Cen X-4 is one of the best studied low-mass neutron star transients in quiescence. Thanks to XMM-Newton large throughput, Cen X-4 was observed at the highest signal to noise ever. This allowed us to disclose rapid (> 100 s), large (45 ± 7 rms in the 10 −4 − 1 Hz range) intensity variability, especially at low energies. In order to highlight the cause of this variability, we divided the data int...

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P - mode observations on α Cen A ⋆

We have made a clear detection of p-mode oscillations in the nearest solar-like G2V star α Cen A with the CORALIE spectrograph on the 1.2-m Swiss telescope at the ESO La Silla Observatory. We report the 5 nights of observation on this star in May 2001 during which 1260 high precision radial velocity measurements were obtained. The power spectrum clearly shows several identifiable peaks between ...

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Archives – draft

The email archives that people accumulate are a dense, complex, and highly personal record of their past interactions. As email becomes increasingly ubiquitous, these include not only their work interactions, but also their relationships with family members, friends, doctors, teachers, etc. However, current mail clients do little to support these archives beyond providing a basic filing and sea...

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ژورنال

عنوان ژورنال: Chemical & Engineering News Archive

سال: 2010

ISSN: 0009-2347,2157-4936

DOI: 10.1021/cen-v088n045.p005