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Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Chinese Academy of SciencesCN1.5k papers
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- Centre National de la Recherche ScientifiqueFR138 papers
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11 papers · 1 filter
New Evidence for the Unified Scheme of BL Lac Objects and Fri Radio Galaxies
J. M. Bai, Myung Gyoon Lee
In this paper, we collect radio and X-ray observations for most Fanaroff-Riley I (FRI) radio galaxies in the Zirbel-Baum radio galaxy sample, and investigate the distribution of th…
Emissive Mechanism on Spectral Variability of Blazars in High Frequencies
Jiancheng Wang, Jirong Mao
The new results of the evolution of the synchrotron peak for Mrk 421 are mostly likely related to the particle acceleration process. In order to account for the above results, we p…
Further detections of OH masers in carbon stars with silicate features
M. Szymczak, R. Szczerba, P. S. Chen
A sample of J-type carbon stars was searched for OH maser emission. The new detection of three OH lines towards two silicate carbon stars is reported. In V778 Cyg, previously known…
Low and intermediate-mass close binary evolution and the initial - final mass relation
Zhanwen Han, Christopher A. Tout, Peter P. Eggleton
Using Eggleton's stellar evolution code, we carry out 150 runs of Pop I binary evolution calculations, with the initial primary mass between 1 and 8 solar masses the initial mass r…
Evaporation: The change from accretion via a thin disk to a coronal flow
Friedrich Meyer, Bifang Liu, Emmi Meyer-Hofmeister
We present a model for a corona above a geometrically thin standard disk around a black hole. This corona is fed by matter from the thin disk which evaporates from the cool layers…
A simple method of determining the Hubble constant
Yi-Ping Qin
Bidirectional relativistic proper motions of radio components of nearby extragalactic sources give a strong constraint on the determination of the Hubble constant . Under the…
Distinguishing RBL-like objects and XBL-like objects with the peak emission frequency of the overall energy spectrum
Yi-Ping Qin, G. Z. Xie, Xue-Tang Zheng
We investigate quantitatively how the peak emission frequency of the overall energy spectrum is at work in distinguishing RBL-like and XBL-like objects. We employ the sample of Gio…
The hardness-duration correlation in the two classes of gamma-ray bursts
Yi-Ping Qin, Guang-Zhong Xie, Sui-Jian Xue +2
The well-known hardness-duration correlation of gamma-ray bursts (GRBs) is investigated with the data of the 4B catalog. We find that, while the hardness ratio and the duration are…
Correlations between various hardness ratios of gamma-ray bursts
Yi-Ping Qin, Guang-Zhong Xie, Xue-Tang Zheng +1
We study correlations between various hardness ratios of gamma-ray bursts (GRBs) and investigate if there are any differences between the two classes of the objects in the distribu…
Black hole X-ray binaries: A new view on soft-hard spectral transitions
F. Meyer, B. F. Liu, E. Meyer-Hofmeister
The theory of coronal evaporation predicts the formation of an inner hole in the cool thin accretion disk for mass accretion rates below a certain value (~ 1/50 of the Eddington ma…
The triple degenerate star WD1704+481
P. F. L. Maxted, T. R. Marsh, C. K. J. Moran +1
WD1704+481 is a visual binary in which both components are white dwarfs. We present spectra of the H-alpha line of both stars which show that one component (WD1704+481.2 = Sandulea…