Answer:
what the
why do ya need dis much info?!?!?!?! AND FOR WHAT!!?!?!?
Explanation:
There would be 4 quarter notes in a 4/4 time signature.
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
brainly.com/question/3527534
#SPJ4
Answer:
i thank that it is all of the above
Explanation:
Answer:
Hey uh...
Explanation:
Hey, I just thought I'd let you know I love you're profile picture. I do believe it's Kastuki Bakugou from My Hero Acedemia or Boku No Hero Acedemia. I'm not even kidding, I just don't know how to tell you this without stealing points as I've literally just recently got an account to this website. Anyways, if I'm wrong about his, sorry. Have a nice day.
