The closer the star the larger The Parallax angle.
The primary mechanism driving the X-ray emission in traditional supergiant high mass X-ray binaries and supergiant fast X-ray transients is the accretion of stellar wind material by a compact object.
We present the first simulation of the fast and dense massive star wind accretion onto a neutron star in this paper, taking into account the effects of the centrifugal and magnetic inhibition of accretion ("gating") caused by the spin and magnetic field of the compact object.
We modeled the nonstationary radiatively generated wind of an O-B supergiant star using a radiative hydrodynamical code, and then we positioned a neutron star with a fixed magnetic field and spin period at a specific distance from the massive companion.
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C. they created portable shelters made from animal hides
How many pets does each of my friends have?
Explanation:
you're comparing multiple different people's pets
Answer:
☆<《<em>HOPE IT WILL HELP YOU</em><em> </em><em>》</em><em>></em><em>☆</em>
Explanation:
seperation is os easy
Seperation is the method in which, if we take a
jar of 1 ml water and add some soil in it after 2or3 hour you will observe that the soil setal down
