![]() |
You entered: stellar wind
![Сформированная звездным ветром туманность RCW 58](https://images.astronet.ru/pubd/2023/02/08/0001878945/Rcw58_Selby_960.preview.jpg)
8.02.2023
Imagine traveling to a star about 100 times as massive as our Sun, a million times more luminous, and with 30 times the surface temperature. Such stars exist, and some are known as Wolf Rayet (WR) stars, named after French astronomers Charles Wolf and Georges Rayet.
![Звезда Вольфа-Райе WR 124: машина звёздного ветра](https://images.astronet.ru/pubd/2014/07/02/0001316384/wr124_hubbleschmidt_960.preview.jpg)
1.07.2014
Some stars explode in slow motion. Rare, massive Wolf-Rayet stars are so tumultuous and hot that they slowly disintegrating right before our telescopes. Glowing gas globs each typically over 30 times more massive than the Earth are being expelled by violent stellar winds.
![Звезда Вольфа-Райе WR 124: машина звездного ветра](https://images.astronet.ru/pubd/2020/03/08/0001629879/wr124_hubbleschmidt_960.preview.jpg)
8.03.2020
Some stars explode in slow motion. Rare, massive Wolf-Rayet stars are so tumultuous and hot that they are slowly disintegrating right before our telescopes. Glowing gas globs each typically over 30 times more massive than the Earth are being expelled by violent stellar winds.
![APOD: 2024 July 22 Б Chamaeleon Dark Nebulas](https://images.astronet.ru/pubd/2024/07/22/0001933873/VeeChamaeleon_Lee_960.preview.jpg)
22.07.2024
Sometimes the dark dust of interstellar space has an angular elegance. Such is the case toward the far-south constellation of Chamaeleon. Normally too faint to see, dark dust is best known for blocking visible light from stars and galaxies behind it.
![Очень большие пузыри в Большом Магеллановом Облаке](https://images.astronet.ru/pubd/2002/10/16/0001180331/superbubbleLMC_umich_big.preview.jpg)
3.07.1996
Why is there a hole in the center of this nebula? A leading explanation is that it is caused by the stellar winds from the stars that live there. Stars - including the Sun - expel electrons, protons, and other charged ions in a steady stream - the stellar wind.
![Темные туманности в Хамелеоне](https://images.astronet.ru/pubd/2022/01/17/0001803439/DarkNebulaVd_HmoRuuth_960.preview.jpg)
17.01.2022
Sometimes the dark dust of interstellar space has an angular elegance. Such is the case toward the far-south constellation of Chamaeleon. Normally too faint to see, dark dust is best known for blocking visible light from stars and galaxies behind it.
![LL Ориона и туманность Ориона](https://images.astronet.ru/pubd/2013/02/03/0001279061/LLOri_hubble_960.preview.jpg)
3.02.2013
This esthetic close-up of cosmic clouds and stellar winds features LL Orionis, interacting with the Orion Nebula flow. Adrift in Orion's stellar nursery and still in its formative years, variable star LL Orionis produces a wind more energetic than the wind from our own middle-aged Sun.
![LL Ориона и туманность Ориона](https://images.astronet.ru/pubd/2006/01/21/0001211023/llori_orion_hst_c14.preview.jpg)
20.01.2006
This esthetic close-up of cosmic clouds and stellar winds features LL Orionis, interacting with the Orion Nebula flow. Adrift in Orion's stellar nursery and still in its formative years, variable star LL Orionis produces a wind more energetic than the wind from our own middle-aged Sun.
![LL Ориона и туманность Ориона](https://images.astronet.ru/pubd/2018/02/18/0001398792/LLOri_hubble_960.preview.jpg)
18.02.2018
Stars can make waves in the Orion Nebula's sea of gas and dust. This esthetic close-up of cosmic clouds and stellar winds features LL Orionis, interacting with the Orion Nebula flow. Adrift...
![NGC 6302: туманность Бабочка](https://images.astronet.ru/pubd/2003/09/09/0001192863/butterfly_vlt_big.preview.jpg)
2.06.1998
The Butterfly Nebula is only thousands of years old. As a central star of a binary system aged, it threw off its outer envelopes of gas in a strong stellar wind. The remaining stellar core is so hot it ionizes the previously ejected gas, causing it to glow.
|
January February March April May June July August |