astro r3

Question 1

Que es el proceso de Kelvin-Helmholtz?

Answer 1

“Epot grav es liberada en la concentracion de un cuerpo
> se convierte en E termica
> aumento
de temperatura”

Question 2

Mecanismo de explosion supernova II

Answer 2

if WD gets >1,4Mo u get a SN

if that results from collapse of Fe core > type II
> N* or BH

(1,4Mo = Chandrasekhar limit)

Question 3

¿Qué dispara el mecanismo de explosión en una supernova de tipo la?

Answer 3

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Question 4

Modelo de formación de sistemas planetarios

parts of HR diagram

Answer 4

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Question 5

Evidencia para el agrupamiento jerárquico

Answer 5

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Question 6

mecanismo explosion SN II

Answer 6

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Question 7

why stars abs lines but quasars em lines?

Answer 7

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Question 8

Evidencia aguj. negro

Answer 8

binarias [but 1 became a BH]
cuasares
“the flickering X-ray emission… of an acc disk”
v* around it (indicates v large mass)

The best evidence of stellar-mass black holes comes from binary star systems in which (1) one star of the pair is not visible, (2) the flickering X-ray emission is characteristic of an accretion disk around a compact object, and (3) the orbit and characteristics of the visible star indicate that the mass of its invisible companion is greater than 3 Mo. A number of systems with these characteristics have been found. Black holes with masses of millions to billions of solar masses are found in the centers of large galaxies.

Question 9

Problemas método v radial

Answer 9

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