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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Answer:
hey leo here!
Explanation:
Making DAW templates might just be the least se//xy part of producing music, but there’s a great logic to getting one made this weekend. When you’re staring down a blank canvas and trying to put a new tune together, you should aim to be in the most creative state possible; searching for plug-ins, creating tracks and setting up routings
hope this helps
Answer: make an effort to remember what has been said
Explanation:
<span>The word talent is from
an Old English word talente, from the Latin talenta, plural of talentum which
means as a unit of weight. From Greek,
it comes from the word talanton which means the name of a sum of currency.</span>
Answer:
I'm almost positive it's
<u>B</u><u>.</u><u> </u><u>lavender</u><u> </u>
Explanation:
neon is not and impressionist is not.
