Pređi na sadržaj

Датотека:LHA 115 - N 76A - Eso0310a.jpg

Sadržaj stranice nije podržan na drugim jezicima
Ovo je datoteka sa Vikimedijine ostave
S Vikipedije, slobodne enciklopedije

Originalna datoteka(4.961 × 4.956 piksela, veličina datoteke: 3,47 MB, MIME tip: image/jpeg)

Opis izmene

Opis
English: This unique image shows AB7, one of the highest excitation nebulae in the Magellanic Clouds (MCs), two satellite galaxies of our own Milky Way. AB7 is a binary star, consisting of one WR-star — highly evolved massive star - and a mid-age massive companion of spectral type O. These exceptional stars have very strong stellar winds: they continuously eject energetic particles — like the "solar wind" from the Sun — but some 10 to 1,000 million times more intensely than our star! These powerful winds exert an enormous pressure on the surrounding interstellar material and forcefully shape those clouds into "bubbles", well visible in the photos by their blue colour. AB7 is particularly remarkable: the associated huge nebula and HeII region indicate that this star is one of the, if not the, hottest WR-star known so far, with a surface temperature in excess of 120,000 degrees ! Just outside this nebula, a small network of green filaments is visible — they are the remains of another supernova explosion.

Credit: ESO

About the Object

Name:	LHA 115-N 76A
Type:	• Local Universe : Star : Grouping : Binary
• Local Universe : Nebula
• Nebulae
Distance:	180000 light years

Colours & filters

Band	Telescope
Optical HeIII 	Very Large Telescope FORS1
Optical OIII 	Very Large Telescope FORS1
Optical H-I 	Very Large Telescope FORS1
.
Izvor http://www.eso.org/public/images/eso0310a/
Autor ESO

Licenciranje

This media was created by the European Southern Observatory (ESO).
Their website states: "Unless specifically noted, the images, videos, and music distributed on the public ESO website, along with the texts of press releases, announcements, pictures of the week, blog posts and captions, are licensed under a Creative Commons Attribution 4.0 International License, and may on a non-exclusive basis be reproduced without fee provided the credit is clear and visible."
To the uploader: You must provide a link (URL) to the original file and the authorship information if available.
w:sr:Krijejtiv komons
autorstvo
Ova datoteka je dostupna pod licencom Creative Commons Autorstvo 4.0 Međunarodna.
Dozvoljeno je:
  • da delite – da umnožavate, raspodeljujete i prenosite delo
  • da prerađujete – da preradite delo
Pod sledećim uslovima:
  • autorstvo – Morate da date odgovarajuće zasluge, obezbedite vezu ka licenci i naznačite da li su izmene napravljene. Možete to uraditi na bilo koji razuman manir, ali ne na način koji predlaže da licencator odobrava vas ili vaše korišćenje.

Natpisi

Dodajte objašnjenje u jednom redu o tome šta ova datoteka predstavlja

Stavke prikazane u ovoj datoteci

prikazuje

status autorskog prava Serbian (transliteracija)

zaštićeno autorskim pravima Serbian (transliteracija)

Istorija datoteke

Kliknite na datum/vreme da biste videli tadašnju verziju datoteke.

Datum/vremeMinijaturaDimenzijeKorisnikKomentar
trenutna00:09, 26. maj 2012.Minijatura za verziju na dan 00:09, 26. maj 2012.4.961 × 4.956 (3,47 MB)Fabian RRRR== {{int:filedesc}} == {{Information |Description={{en|1=This unique image shows AB7, one of the highest excitation nebulae in the Magellanic Clouds (MCs), two satellite galaxies of our own Milky Way. AB7 is a binary star, consisting of one WR-star —...

Sledeća stranica koristi ovu datoteku:

Globalna upotreba datoteke

Drugi vikiji koji koriste ovu datoteku:

Metapodaci