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Topic: NGC 5128

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	NGC 5128 (Centaurus A) in Centaurus
		NGC 5128 is a unique galaxy in that it has a distinct dust lane girdling its diameter.
		It is believed to be the remnant of a spiral galaxy that was merged into the elliptical galaxy NGC 5128.
		NGC 5128 is a strong source of radio frequency radiation.
	jthommes.com /Astro/NGC5128.htm (287 words)

	Centaurus A (NGC 5128)
		The second strongest extragalactic radio source in the sky (after Cygnus A) and the nearest radio galaxy to the Milky Way; it lies in the constellation Centaurus, 13 to 15 million light-years away in the M83 group of galaxies.
		Cen A’s optical counterpart, discovered by James Dunlop in 1826, is an unusual elliptical galaxy (NGC 5128) bisected by a dark circumgalactic dust belt that appears to be debris from a merger between the elliptical and at least one spiral galaxy over the past few billion years.
		The most active radio emission, however, is associated with Cen A’s compact core which is the foremost example of a radio-loud active galactic nucleus and, at only 10 light-days across, the smallest known extragalactic radio source.
	www.daviddarling.info /encyclopedia/C/Centaurus_A.html (275 words)

	NGC 5128 - Centaurus A
		NGC 5128, Centaurus A, Cen A, Bennett 60
		Cen A, also known as NGC 5128, is also unusual compared to an average elliptical galaxy because it contains a higher proportion of young blue stars and is a very strong source of radio emission.
		Centauraus A is the closest active galaxy: together with NGC 4945 and M 83, it forms part of a small group of galaxies 13 million lightyears away.
	www.astrosurf.com /antilhue/ngc5128_rc.htm (202 words)

	Wszechświat w odległości 100 milonów lat świetlnych - Supergromada w Pannie (Supergromada Lokalna)
		Grupa w Rzeźbiarzu jest najbliższą grupą galaktyk dla naszego Układu Lokalnego i jest zdominowana przez pięć galaktyk; cztery spiralne- NGC 247, 253, 300 i 7793 oraz jedną nieregularną - NGC 55.
		Jest to sąsiednia grupa galaktyk w Centaurze (Centaurus), zdominowana przez dwie galaktyki spiralne M83 i NGC 4945 oraz dużą soczewkowatą NGC 5128.
		NGC 5128 to jedna z najjaśniejszych blikskich nam galaktyk, a zarazem jest to poteżne źródło fal radiowych [znane radioastronomom jako Centaur A (Centaurus A)].
	wszechswiat.astrowww.pl /virgo.html (984 words)

	NGC 5128 (Centaurus A)
		NGC 5128 (Centaurus A) A radio galaxy, NGC 5128 (Centaurus A) AAO image reference AAT 7.
		The field of NGC 5128 (Centaurus A, landscape format)
		The field of NGC 5128 (Centaurus A, portrait format)
	www.aao.gov.au /images/captions/aat007.html (240 words)

	NGC 5128 dust lane
		The Dust Lane of NGC 5128 (Centaurus A)
		The dark band is probably the remains of a dusty spiral galaxy which is being absorbed by the giant elliptical.
		NGC 5128 Gx 13 25.5 -43 01 s Cen 18.27.0 !!, vB, vL, vmE 122deg, bifid
	www.aao.gov.au /images/captions/aat052.html (258 words)

	The Universe within 100 million Light Years - The Virgo Supercluster
		The Sculptor group is the nearest group of galaxies to the Local Group and is dominated by five galaxies, four spiral - NGC 247, 253, 300 and 7793 and one irregular - NGC 55.
		This is a neighbouring group of galaxies in Centaurus and is dominated by the two spiral galaxies M83 and NGC 4945 and the large lenticular galaxy NGC 5128.
		NGC 5128 is one of the brightest nearby galaxies and it is a powerful source of radio waves (radio astronomers call the galaxy Centaurus A).
	www.atlasoftheuniverse.com /virgo.html (1108 words)

	NGC 5128 - Vikipedio
		NGC 5128, ESO 270-9, IRAS13225-4245, MCG -7-28-1, AM 1322-424, ARP 153, PRC C-45, PGC 46957
		NGC 5128 (aliaj indikoj — ESO 270-9, IRAS13225-4245, MCG -7-28-1, AM 1322-424, ARP 153, PRC C-45, PGC 46957) estas galaksio en konstelacio Centaŭro.
		Ĉi tiu artikolo pri "NGC 5128" ankoraŭ estas ĝermo pri kosma objekto.
	eo.wikipedia.org /wiki/NGC_5128#Vidu_anka.C5.AD_jenon: (159 words)

	Galaxy Centaurus A / NGC 5128
		In 1949, NGC 5128 was found to be a powerful radio galaxy by early radio astronomers (which was first suggested by John Bolton, Gorden Stanley, and Bruce Slee in Nature, I64, 101, 1949; according to Baade and Minkowski, 1954, pp.
		It then shared the additional designation of Centaurus A, which had been determined to be the brightest radio source in the direction of (13:25:28-43:1:11 J2000; and 13:25:27.6-43:1:8.8, ICRS 2000) of Constellation Centaurus, the Centaur, north of globular cluster Omega Centauri (NGC 5139) and west of Mu Centauri -- map.
		Found to be the closest "radio-loud" galaxy to the Solar System (José Luis Sérsic, 1960), its radio emissions comes from two giant lobes that extend over a million light-years (ly), roughly at right angles to the galaxy's dark dust band.
	www.solstation.com /x-objects/cent-a.htm (1484 words)

	Unusual and extreme stars (Site not responding. Last check: 2007-11-01)
		The Tarantula Nebula, before supernova SN1987A, in the Large Magellanic Cloud
		Supernova 1986g in NGC 5128 (Cen A) Supernova 1986g in NGC 5128 (Cen A) The nebula around R Aquarii, a symbiotic star
		IC 2220, deep image of the Toby Jug nebula
	www.aao.gov.au /images/general/stars.html (53 words)

	MPE Jahresbericht 2000 - IV / MPE Annual Report 2000 - IV
		Genzel, A. Sternberg and H. Netzer: Infrared Spectroscopy of NGC 1068: Probing the Obscured Ionizing AGN Continuum.
		Schinnerer, E., A. Eckart and L.J. Tacconi: Distribution and Kinematics of the Circumnuclear Molecular Gas in the Seyfert 1 Galaxy NGC 3227.
		Anders, L.E. Tacconi-Garman and N. Thatte: Stellar Dynamics and the Implications on the Merger Evolution in NGC 6240.
	www.mpe.mpg.de /JB2000/publications.html (11123 words)

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