Answer: I have a favorite rapper
Explanation:
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.
To learn more about Parallax Star here
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Answer:
Go to the IMB website and look up "Philip Zimbardo's Stanford Prison Experiment" and you can look at the cast members list.
Explanation:
This is one way of doing it. I cannot put the website because of brainly's rules.
Answer:
one that shows originality and versatility
Explanation:
Be sure to include work that demonstrates your ability to produce deliverables in diverse industries. You may also want to add some personal flair to your portfolio by including a piece of work that shows off your skills and your passion for graphic design.
