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OTSI VARASEMAID OSASID

Otsi kanali 17. Galactic Mass Distribution and Galaxy Structure viimaseid osasid.

MUUD EPISOOD SELLES PODCASTIS

Transcript: It’s a great challenge to determine the true incidence of binary and multiple star systems. The nearest stars are well observed, but it’s a very small sample. As we go to more distant stars a faint companion might not be detectable. Spectroscopic binaries are biased towards small sep…

Supernova

Transcript: Consider a binary system where a giant or a supergiant star is in orbit around a white dwarf and where a mass transfer between the lobes pushes the white dwarf over the Chandrasekhar limit. At this point the white dwarf collapses catastrophically to form either a neutron star or a blac…
Transcript: How does mass transfer occur in a close binary pair? The Roche surface or lobes define the region of space where gas is bound to one or both stars. If either star becomes a giant the outer layers swell to fill the lobe, and the teardrop shape becomes the actual surface of the star. I…

Nova

Transcript: Consider a binary pair where the more massive star has expanded to fill its Roche lobe, and the smaller star is a white dwarf of nearly 1.4 solar masses. As the massive star dumps hydrogen onto the white dwarf the gas is compressed, rapidly heated, and it ignites nuclear reactions that…
Vastutamatussäte: Sellele lehele manustatud taskuhäälingusaade ja kunstiteosed pärinevad Dr. Christopher D. Impey, Professor, Astronomy-lt, mis on selle omaniku omand ja ei ole seotud ettevõttega Listen Notes, Inc.