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Дата изменения: Sat Oct 14 21:07:48 2000
Дата индексирования: Mon Oct 1 20:13:58 2012
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Поисковые слова: rigel
starse

The stars.

The Stars - are the shining (plasma) spheres like the Sun. Generated from the gas and dust medium due to the gravitational instability. The star’s masses M are from 0,04 to 60 л¤, luminary (L) from 0,5 to hundreds thousand L¤ (see later). The stars are classified by their luminance mass, the surface temperature, chemical composition, the spectrum peculiarities. On the definite step of the stars evolution the stars come through the period of nonstationarity (see "nonstationary stars"). Depending on mass the stars become at the end of evolution the white dwarfs or the neutron stars or the black holes.

Sirius
Sirius

The Sun
The Sun

Aldebaran
Aldebaran

Rigel
Rigel

The blowing stars.

The supernew stars.

Supernew star are unexpectedly bursting star, the power of which during the burst is from 10^40 erg/s and higher. The gravitational collapse brings these bursts.

 

The nebula Veil
The nebula Veil

The nebula Loop of the Swan
The nebula Loop of the Swan

The nebula Loop of the Swan
The nebula Loop of the Swan

 

The supernew SN 1987A
The supernew SN 1987A

The crab nabula
The crab nebula

The doublestars.

Object SS 433
Object SS 433