Exosat observations of H2252-035: Pulse phase and orbital phase dependent low energy absorption and iron line emission

1987 ◽  
Vol 130 (1-2) ◽  
pp. 281-292 ◽  
Author(s):  
W. Pietsch ◽  
W. Voges ◽  
E. Kendziorra ◽  
M. Pakull
1987 ◽  
Vol 93 ◽  
pp. 281-292
Author(s):  
W. Pietsch ◽  
W. Voges ◽  
E. Kendziorra ◽  
M. Pakull

AbstractThe 805 sec pulsing X-ray source H2252−035 has been observed for 7 h on September 14/15 and on September 17, 1983 in X-rays with the low energy telescope and the medium energy detectors of EXOSAT. While below 2 keV the semiamplitude of the 805 s pulses is ~ 100% in the 2.3–7.9 keV band it is only ~ 40%. X-ray dips that are more pronounced in low energies occur simultaneously with the orbital minimum of the optical light curve. The medium energy spectra during dips with respect to the non dip spectrum can be explained by just enhanced cold gas absorption of an additional absorbing column of 2 1022 cm−2. Model spectra for the 805 s minimum have to include a strong iron emission line at 6.55 keV with an equivalent width of 3 keV in addition to a reduced continuum intensity (radiating area) and enhanced low energy absorption.


2017 ◽  
Author(s):  
Kumiko Nobukawa ◽  
Masayoshi Nobukawa ◽  
Shigeo Yamauchi ◽  
Hideki Uchiyama ◽  
Katsuji Koyama

2021 ◽  
Vol 57 (11) ◽  
pp. 1316-1319
Author(s):  
Yohei Adachi ◽  
Takanori Nomura ◽  
Shion Tazuhara ◽  
Hiroyoshi Naito ◽  
Joji Ohshita

A new boron-embedded bistricyclic aromatic ene (BAE) exhibits a low-energy absorption and obvious n-type semiconducting character with moderate electron field-effect mobilities in OFETs.


2006 ◽  
Vol 453 (1) ◽  
pp. L13-L16 ◽  
Author(s):  
L. Miller ◽  
T. J. Turner ◽  
J. N. Reeves ◽  
I. M. George ◽  
D. Porquet ◽  
...  
Keyword(s):  

2020 ◽  
Vol 12 (5) ◽  
pp. 168781402092413
Author(s):  
Lai Hu ◽  
Jun Zha ◽  
Yaolong Chen

This study conducted an investigation on transverse quasi-static three-point loading on a circular aluminum tube and its characteristic plastic failure and energy-absorption behaviors. The thin wall thickness of the aluminum tube, the various diameter and thickness ratios ( D/ t) of the tube, and the tube length are important control parameters. Experimental data for different span length and thickness ratios of the tube were characterized and correlated to its plastic collapse behavior. A simulation model by computational analysis using ANSYS was also conducted as a comparative study. The results of the study found that transverse three-point bend loading (ASTM F290) of a circular aluminum tube underwent different stages of deformation, from initial pure crumpling to crumpling and bending, and finally, structural rupture. The results of master curve analysis found that regions of high energy absorption and low energy absorption can be classified with respect to the characteristic tubular deformation. High energy absorption deformation is correlated with a short span length and higher D/ t ratio, and vice versa for low energy absorption deformation of the circular aluminum tube. Simulation analysis also predicted similar characteristic trends of deformation behavior in the experiment, with a less than 3% average coefficient of variation.


1978 ◽  
Vol 226 ◽  
pp. 282 ◽  
Author(s):  
H. L. Kestenbaum ◽  
W. H.-M. Ku ◽  
K. S. Long ◽  
E. H. Silver ◽  
R. Novick

1973 ◽  
Vol 184 ◽  
pp. L1 ◽  
Author(s):  
P. J. Serlemitsos ◽  
E. A. Boldt ◽  
S. S. Holt ◽  
R. Ramaty ◽  
A. F. Brisken
Keyword(s):  
X Ray ◽  

1982 ◽  
Vol 97 ◽  
pp. 97-106 ◽  
Author(s):  
C. Jones ◽  
W. Forman

The earliest Uhuru observations showed that cluster X-ray sources were not associated with single individual galaxies but were extended sources (Gursky et al. 1971, Kellogg et al. 1972, and Forman et al. 1972). The detection of iron line emission from X-ray spectroscopic observations (Mitchell et al. 1976 and Serlemitsos et al. 1977) showed both that the dominant X-ray emission process was thermal bremsstrahlung and that the gas had been processed through stellar systems before being injected into the intracluster medium.


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