![Numerical Calculation of Magnetobremsstrahlung Emission and](http://s1.studyres.com/store/data/015318877_1-5d504a1d170e3c995c85195baa9ec7f4-300x300.png)
L95 IRON-RICH EJECTA IN THE SUPERNOVA
... the Fe and Si-group elements as a function of radius in the core region. For simplicity, we assume a spherical geometry for the deprojection. If the true three-dimensional shape of the core region were ellipsoidal, then our mass estimates would be some 13% higher (prolate) or lower (oblate). We assu ...
... the Fe and Si-group elements as a function of radius in the core region. For simplicity, we assume a spherical geometry for the deprojection. If the true three-dimensional shape of the core region were ellipsoidal, then our mass estimates would be some 13% higher (prolate) or lower (oblate). We assu ...
Adhesion of Oral Streptococci from a Flowing
... Busscher et a / . (1986) noted that reversible adhesion was associated with a positive AF,,, while irreversible adhesion was associated with negative AFadhvalues. Most bacterial adhesion experiments have been done under more or less static conditions, with poorly controlled hydrodynamics, irreproduc ...
... Busscher et a / . (1986) noted that reversible adhesion was associated with a positive AF,,, while irreversible adhesion was associated with negative AFadhvalues. Most bacterial adhesion experiments have been done under more or less static conditions, with poorly controlled hydrodynamics, irreproduc ...
XMM-Newton discovery of 7 s pulsations in the isolated neutron star
... We started the timing analysis using the data of the pn camera and selecting the energy range 0.15-1.2 keV. Due to the very soft spectrum of RX J1856.5–3754, practically no source photons are detected at higher energies. We used a circular extraction region centered at the source position and with r ...
... We started the timing analysis using the data of the pn camera and selecting the energy range 0.15-1.2 keV. Due to the very soft spectrum of RX J1856.5–3754, practically no source photons are detected at higher energies. We used a circular extraction region centered at the source position and with r ...
This is the Title - Astronomy at Swarthmore College
... those due to density. The high-density shells of dust primarily affect the amount of UV light that reaches each radius from the external field. While the higher densities also increase the collisional reaction rates, densities at these radii are small enough to make the effect negligible. Thus, the ...
... those due to density. The high-density shells of dust primarily affect the amount of UV light that reaches each radius from the external field. While the higher densities also increase the collisional reaction rates, densities at these radii are small enough to make the effect negligible. Thus, the ...
SRC and the fate of cold neutron stars
... Theoretical conclusion: distribution of nucleons within gas of strongly interacting nucleons even at zero temperature is different from step function. Occupation number for a nucleon within Fermi surface <0.7 at nuclear density. ...
... Theoretical conclusion: distribution of nucleons within gas of strongly interacting nucleons even at zero temperature is different from step function. Occupation number for a nucleon within Fermi surface <0.7 at nuclear density. ...
Turbulent molecular gas and star formation in the shocked
... range) were affected by spurious spikes, likely due to the electronics of other receivers that were powered-on at the time of the observations). Therefore, a sigma-clipping has been applied. By scanning across all spectra, the sigma associated with each channel, σc , is determined. The data is flagg ...
... range) were affected by spurious spikes, likely due to the electronics of other receivers that were powered-on at the time of the observations). Therefore, a sigma-clipping has been applied. By scanning across all spectra, the sigma associated with each channel, σc , is determined. The data is flagg ...
Cross-sectional area and intensity variations of sausage modes⋆
... expected φδφB,0B = 0. Note that the terms in Eqs. (12)–(14) before J1 (nR)/nR are the same as the terms in Eqs. (9)–(11) before I1 (κR)/κR. We shall use I1 to indicate the first term in Eq. (9), I2 to indicate the second term in Eq. (9), and S 1 to indicate the first term in Eq. (10). Looking at Eqs ...
... expected φδφB,0B = 0. Note that the terms in Eqs. (12)–(14) before J1 (nR)/nR are the same as the terms in Eqs. (9)–(11) before I1 (κR)/κR. We shall use I1 to indicate the first term in Eq. (9), I2 to indicate the second term in Eq. (9), and S 1 to indicate the first term in Eq. (10). Looking at Eqs ...
Microplasma
![](https://commons.wikimedia.org/wiki/Special:FilePath/PaschenCurve.jpg?width=300)
Microplasmas are plasmas of small dimensions, ranging from tens to thousands of micrometers. They can be generated at a variety of temperatures and pressures, existing as either thermal or non-thermal plasmas. Non-thermal microplasmas that can maintain their state at standard temperatures and pressures are readily available and accessible to scientists as they can be easily sustained and manipulated under standard conditions. Therefore, they can be employed for commercial, industrial, and medical applications, giving rise to the evolving field of microplasmas.