Search results for " X-rays"

showing 4 items of 234 documents

Spectral analysis of the dipping LMXB system XB 1916-053

2019

Context: XB 1916-053 is a low mass X-ray binary system (LMXB) hosting a neutron star (NS) and showing periodic dips. The spectrum of the persistent emission was modeled with a blackbody component having a temperature between 1.31 and 1.67 keV and with a Comptonization component with an electron temperature of 9.4 keV and a photon index $\Gamma$ between 2.5 and 2.9. The presence of absorption features associated with highly ionized elements suggested the presence of partially ionized plasma in the system. Aims: In this work we performed a study of the spectrum of XB 1916-053, which aims to shed light on the nature of the seed photons that contribute to the Comptonization component. Methods: …

stars: individual: XB 1916-053Absorption spectroscopyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesContext (language use)AstrophysicsX-rays: general01 natural sciencesSpectral lineformation identification Line neutron Stars Stars: individual: XB 1916-053 X-rays: binaries X-rays: generalX-rays: binariesstars: neutron0103 physical sciencesBlack-body radiationAbsorption (logic)010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsAstronomy and AstrophysicsNeutron starAbsorption edgeSpace and Planetary ScienceElectron temperatureline: formationAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]line: identification
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The structure of coronal plasma in active stellar coronae from density measurements

2005

We have analyzed high-resolution X-ray spectra of a sample of 22 active stars observed with the High Energy Transmission Grating Spectrometer (HETGS) on Chandra in order to investigate their coronal plasma density, using the lines of the He-like ions O VII, Mg XI, and Si XIII. Si XII lines in all stars of the sample axe compatible with the low-density limit (i.e. n(e) = 10(30) erg/s); O VII lines yield much lower densities of a few 10(10) cm(-3). Our results indicate that the "hot" and "cool" plasma resides in physically different structures. Our findings imply remarkably compact coronal structures, especially for the hotter (similar to 7 MK) plasma emitting the Mg xi lines characterized by…

sun : coronastars : activitySettore FIS/05 - Astronomia E AstrofisicaX-rays : starlate-typeactivity; coronae; late-type; sun : corona; X-rays : stars; spectroscopic plasma diagnostics [stars]coronaespectroscopic plasma diagnostics
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Chandra study of the eclipsing M dwarf binary, YY Gem

2012

The eclipsing M dwarf binary system, YY Gem, was observed using Chandra covering 140 ks (2Prot) in total, split into two even exposures separated by 0.76 d (0.94 Prot). The system was extremely active: three energetic flares were observed over the course of these observations. The flaring and non-flaring states of the system are analysed in this paper. The activity level increased between the first and second observations even during the quiescent (non-flaring) phases. An analysis of the dynamics of the X-ray-emitting plasma suggests that both components are significantly active. Contemporaneous Hα spectra also suggest that both components show similar levels of activity. The primary star i…

techniques: spectroscopic binaries: eclipsing stars: coronae stars: flare stars: magnetic field X-rays: starsspectroscopic binaries: eclipsing stars: coronae stars: flare stars: magnetic field X-rays: stars [techniques]Settore FIS/05 - Astronomia E Astrofisica
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Soft X-ray Tomography Reveals HSV-1-Induced Remodeling of Human B Cells.

2022

Upon infection, viruses hijack the cell machinery and remodel host cell structures to utilize them for viral proliferation. Since viruses are about a thousand times smaller than their host cells, imaging virus-host interactions at high spatial resolution is like looking for a needle in a haystack. Scouting gross cellular changes with fluorescent microscopy is only possible for well-established viruses, where fluorescent tagging is developed. Soft X-ray tomography (SXT) offers 3D imaging of entire cells without the need for chemical fixation or labeling. Here, we use full-rotation SXT to visualize entire human B cells infected by the herpes simplex virus 1 (HSV-1). We have mapped the temporo…

viruksetisäntäsolutBioengineeringmikroskopiainfektiotMicrobiologyX-ray tomography; soft X-rays; infection imaging; HSV-1; cell mapping; cryo imagingherpes simplex -virusCapsidsoft X-raystomografiaVirologyHumans2.2 Factors relating to the physical environment2.1 Biological and endogenous factorsAetiologyherpesviruksetTomographycryo imagingHerpesvirus 1herpesinfection imagingHSV-1solutInfectious Diseasesröntgenkuvauscell mappingX-RaySexually Transmitted InfectionsInfectionX-ray tomographysolubiologiaHuman
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