Pinwheel nebula

Pinwheel nebula

A pinwheel nebula is a "nebulous region" in the shape of a pinwheel.

piral galaxies

The term 'Pinwheel nebula' is an antiquated misnomer used by observers before Edwin Hubble realized that these spiral shaped nebulae were actually 'island universes'.

Wolf-Rayet nebulae

Some Wolf-Rayet stars are surrounded by pinwheel nebulae. These nebulae are formed from the dust that is spewed out of a binary star system. The stellar winds of the two stars collide and form two dust lanes that spiral outward with the rotation of the system.

External links

* [http://www.physics.usyd.edu.au/~gekko/wr104.html] Some Wolf-Rayet stars in binaries are close enough that we can image a rotating "pinwheel nebula" showing the dust generated by colliding winds in the binary system, from Aperture Masking Interferometry observations.
* [http://www.spacetelescope.org/news/html/heic0602.html Pinwheel Galaxy from ESA/Hubble]


Wikimedia Foundation. 2010.

Игры ⚽ Нужно решить контрольную?

Look at other dictionaries:

  • Pinwheel Galaxy — For other uses, see Pinwheel Galaxy (disambiguation). Pinwheel Galaxy Observation data (J2000 epoch) Constellation …   Wikipedia

  • Wolf-Rayet nebula — A Wolf Rayet nebula is a nebula which surrounds a Wolf Rayet star. A subtype of a WR nebula is the Pinwheel nebula.There are different types of WR nebula, based on their formation mechanism: * HII regions * ejecta type nebulae * wind blown… …   Wikipedia

  • Wolf–Rayet star — Hubble Space Telescope image of nebula M1 67 around Wolf–Rayet star WR 124 Wolf–Rayet stars (often referred to as WR stars) are evolved, massive stars (over 20 solar masses initially), which are losing mass rapidly by means of a very strong… …   Wikipedia

  • Wolf-Rayet star — Wolf Rayet stars (often referred to as WR stars) are evolved, massive stars (over 20 solar masses), which are losing mass rapidly by means of a very strong stellar wind, with speeds up to 2000 km/s. While our own Sun loses approximately 10−14 of… …   Wikipedia

  • WR 104 — Starbox begin name=WR 104Starbox observe epoch=2000 [http://simbad.u strasbg.fr/simbad/sim id?protocol=html Ident=wr104 SIMBAD query result ] ] ra=RA|18|02|04.07 dec=DEC| 23|37|41.2 appmag v= constell=Starbox character class= WCv+Starbox… …   Wikipedia

  • Colliding-wind binary — A colliding wind binary is a binary star system in which the two members are massive stars that emit powerful, radiatively driven stellar winds. The location where these two winds collide produces a strong shock front that can cause radio, X ray… …   Wikipedia

  • Coma Berenices — For other uses, see Coma Berenices (disambiguation). Coma Berenices Constellation List of stars in Coma Berenices Abbreviation Com Gen …   Wikipedia

  • Liste von Eigennamen von Deep-Sky-Objekten — Diese Seite ist eine Liste von Eigennamen von Deep Sky Objekten. Inhaltsverzeichnis 1 Sternhaufen und Sterngruppen 2 Interstellare Materie 3 Galaxien, Galaxiengruppen und haufen 4 Weitere astron …   Deutsch Wikipedia

  • Triangulum Galaxy — Messier 33 Observation data (J2000 epoch) Pronunciation /traɪˈæŋɡjʉləm/ …   Wikipedia

  • Pierre Méchain — Born 16 August 1744(1744 08 1 …   Wikipedia

Share the article and excerpts

Direct link
Do a right-click on the link above
and select “Copy Link”