نتایج جستجو برای: the line 7219

تعداد نتایج: 16098329  

2000
John P. Hughes Cara E. Rakowski

In this Letter we use the unprecedented spatial resolution of the Chandra X-Ray Observatory to carry out, for the first time, a measurement of the post-shock electron temperature and proper motion of a young SNR, specifically to address questions about the post-shock partition of energy among electrons, ions, and cosmic rays. The expansion rate, 0.100% ± 0.025%yr, and inferred age, ∼1000 yr, of...

پایان نامه :وزارت علوم، تحقیقات و فناوری - دانشگاه فردوسی مشهد - دانشکده ادبیات و علوم انسانی دکتر علی شریعتی 1389

the purpose of this study is to investigate the relationships between teachers’ immediacy behaviors and iranian students’ willingness to talk in english classes. analysis of the results from willingness to talk scale represents a relatively high level of willingness to talk in english classrooms among iranian language learners. the total mean score of students’ willingness to talk was 66.3 ou...

Journal: :The Astrophysical Journal 2021

Abstract The centroid energy of the Fe K α line has been used to identify progenitors supernova remnants (SNRs). These investigations generally considered derived from spectrum entire remnant. Here we use XMM-Newton data investigate in 6 SNRs: 3C 397, N132D, W49B, DEM L71, 1E 0102.2-7219, and Kes 73. In 73 fail detect any emission. We report a tentative first detection emission SNR L71 with con...

پایان نامه :وزارت علوم، تحقیقات و فناوری - دانشگاه شهید چمران اهواز - دانشکده ادبیات و علوم انسانی 1389

methodology non-native participants in this study were sixty ba students majoring in english literature and teaching english as a foreign language at khayyam university of mashhad. they were senior students, between 21 to 24 years old, who had studied english for at least three and a half years and had passed several courses including grammar, reading, conversation, and writing. this was assum...

2003
K. A. Flanagan C. R. Canizares D. Dewey J. C. Houck A. C. Fredericks M. L. Schattenburg T. H. Markert D. S. Davis

Chandra High Energy Transmission Grating Spectrometer observations of the supernova remnant 1E 0102.2-7219 in the Small Magellanic Cloud reveal a spectrum dominated by X-ray emission lines from hydrogen-like and helium-like ions of oxygen, neon, magnesium and silicon, with little iron. The dispersed spectrum shows a series of monochromatic images of the source in the light of individual spectra...

Journal: :International Journal of Low-carbon Technologies 2023

Abstract This paper carried out the environmental and economic evaluation for hydrogen storage technologies on sedan with Type 3 4 high-pressured cryogenic vessels based life cycle analysis (LCA) method. It is found that vessel manufacture emits minimum greenhouse gas (GHG) 5539 kgCO2 eq, which lower than of 7219 eq 135 000 in their whole cycle. The shows high-pressure has lowest cost 10.4 US$/...

Journal: :The Astrophysical Journal 2021

We present new proper motion measurements of optically emitting oxygen-rich knots supernova remnant 1E 0102.2-7219 (E0102), which are used to estimate the remnant's center expansion and age. Four epochs high resolution Hubble Space Telescope images spanning 19 yr were retrieved analyzed. found a robust alpha=1:04:02.48 delta=-72:01:53.92 (J2000) with 1-sigma uncertainty 1.77 arcseconds using 45...

2008
Karin Sandstrom Alberto Bolatto Snežana Stanimirović J. D. Smith Joshua D. Simon Adam Leroy

The quantity and composition of dust produced in core-collapse supernovae is a matter of much debate. Observations of dust around quasars at high redshift have been explained via models invoking efficient dust production, with typical yields of 0.1-1 M⊙ of dust per supernova. Observations of supernovae and their remnants, however, have yet to provide evidence for efficient dust production. Obse...

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