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Topic: NGC 604

	Firestorm Of Star Birth Seen In A Local Galaxy
		This festively colorful nebula, called NGC 604, is one of the largest known seething cauldrons of star birth in a nearby galaxy.
		NGC 604 lies in a spiral arm of the nearby galaxy M33, located about 2.7 million light-years away in the direction of the constellation Triangulum.
		NGC 604 itself can be seen in a small telescope, and was first noted by the English astronomer William Herschel in 1784.
	www.spacedaily.com /news/extrasolar-03u.html (651 words)

	NationMaster - Encyclopedia: List of messier objects (Site not responding. Last check: 2007-10-29)
		NGC 4414, a typical spiral galaxy in the constellation Coma Berenices, is about 56,000 light years in diameter and approximately 60 million light years distant.
		NGC 6543, the Cats Eye Nebula A planetary nebula is an astronomical object consisting of a glowing shell of gas and plasma formed by certain types of stars at the end of their lives.
		The Spindle Galaxy (NGC 5866), a lenticular galaxy in the Draco constellation.
	www.nationmaster.com /encyclopedia/List-of-messier-objects (5167 words)

	M33text (Site not responding. Last check: 2007-10-29)
		Close examination of the inner structure of NGC 604 reveals a large number of shells, filaments, and arches formed by the stellar winds of 200 O type giants plus several Wolf-Rayet stars.
		NGC 604 is powered by an extended OB association lacking a central concentrated core like R136 in 30 Doradus.
		The massive stars of NGC 604 are scattered over a large area spanning the entire nebula and are 100 times less concentrated than R136.
	www.robgendlerastropics.com /M33text.html (0 words)

	Hubble Space Telescope, Thumbnail Views page 7
		NGC 4622, "Backwards," Spiral Galaxy: To the surprise of astronomers, this galaxy appears to be rotating backwards.
		NGC 6369, Little Ghost Nebula: This object is known to amateur astronomers as the "Little Ghost Nebula," because it appears as a small, ghostly cloud surrounding the faint, dying central star.
		NGC 6369 lies in the direction of the constellation Ophiuchus, at a distance estimated to be between about 2,000 and 5,000 light-years from Earth.
	www.laughtergenealogy.com /bin/hubble/thumbs07.html (1871 words)

	Universe Today - Hubble's View of Starbirth
		NGC 604 is 2.7 million light-years away in the constellation Triangulum.
		This festively colorful nebula, called NGC 604, is one of the largest known seething cauldrons of star birth in a nearby galaxy.
		Color filters were used to isolate light emitted by hydrogen, oxygen, nitrogen, and sulfur atoms in the nebula and ultraviolet, visible and infrared light from the stars within NGC 604 and the nearby spiral arms of M33.
	www.universetoday.com /am/publish/hubble_ngc604.html (579 words)

	Space Today Online - Deep Space - Telescopes - Hubble Space Telescope - beautiful views
		NGC 604 is a hotbed of starbirth in an arm of the spiral galaxy known as Triangulum galaxy or M33.
		NGC 5307 nebula in the constellation Centaurus spins like a pinwheel as blobs of gas are ejected from each side of the central star.
		NGC 7027 was a medium-mass star like our Sun before it began casting off clouds of gas and glowing material in spectacular death throes.
	www.spacetoday.org /DeepSpace/Telescopes/GreatObservatories/Hubble/HubbleBeauty.html (1406 words)

	Observations in TRIANGULUM
		NGC 684 Pretty faint, pretty large, elongated 2 X 1 in PA 90 and brighter in the middle at 135X.
		NGC 751 is separated from 750 even at this power, but going to 165X does help split this galaxy pair.
		NGC 959 Pretty faint, pretty large, elongated 1.5 X 1 in PA 90 and somewhat brighter in the middle at 100X.
	www.saguaroastro.org /content/obsnotes/TRIANGULUM.htm (0 words)

	NGC 604 in M33
		This is a Hubble Space Telescope image (right) of a vast nebula NGC 604 in the Triangulum galaxy M33.
		At the heart of NGC 604 are over 200 hot stars, much more massive than our Sun (15 to 60 solar masses).
		NGC 604 was first cataloged by William Herschel on September 11, 1784, who assigned it the number H III.150.
	www.seds.org /messier/more/m033_n604.html (0 words)

	RE: (IAAC) Obj: NGC 604 - Inst: 200mm Newtonian (Site not responding. Last check: 2007-10-29)
		The big difference between the Gum and NGC 604 nebulae is that the Gum is probably a very old supernova remnant (expanding), while NGC 604 is a stellar nursery in a contracting gas cloud, the same as M 42 or M 8.
		Hundreds of young bright stars in NGC 604 illuminate the cloud to a much higher surface brightness than the Gum.
		If NGC 604 were to be moved to our neighborhood in our galaxy it would be quite spectacular.
	www.visualdeepsky.org /netastrocatalog-announce/msg02620.html (276 words)

	Fotos do Hubble - Chamas do Nascimento de uma Estrela Vistas em uma Galáxia Local
		A NGC 604 é parecida com as regiões familiares de nascimento de estrelas em nossa Via Láctea, tais como a Nebulosa de Órion, mas é muito maior e contém muito mais estrelas recém-formadas.
		As estrelas brilhantes na NGC 604 são extremamente jovens pelos padrões astronômicos, tendo sido formadas há apenas 3 milhões de anos.
		A NGC 604 pode ser vista através de pequenos telescópios, e foi primeiro observada pelo astrônomo inglês William Herschel em 1784.
	www.sentandoapua.com.br /astronomia/h55.htm (540 words)

	Hubble Heritage
		This image of NGC 604 was taken in several different wide-band (W) and narrow-band (N) filters with the Wide Field Planetary Camera 2 onboard Hubble.
		NGC 604 contains more than 200 hot, bright stars within a cloud that is nearly 1,300 light-years across.
		A press release image of NGC 604 was released in 1996 (STScI PRC96-27) which included only a few of the narrow-band filters.
	heritage.stsci.edu /2003/30/supplemental.html (0 words)

	Pinwheel Galaxy M33
		This image of the nearby spiral galaxy M33 (NGC 598) in Triangulum is from a 30-minute V-band exposure obtained with the UA 0.4m telescope, spanning a region almost 0.3 by 0.5 degree.
		NGC 604 is among the brightest such regions in the entire Local Group, comparable in output to the Tarantula Nebula and perhaps our own NGC 3603.
		For historical continuity, here is teh first image posted here some years ago: The nuclear region of the nearby spiral M33 (NGC 598), imaged in the V band using the Lowell Observatory 1.1-meter telescope.
	www.astr.ua.edu /gifimages/m33.html (0 words)

	2MASS Atlas Image Gallery
		NGC 205 is peculiar in that evidence exists for recent star formation in what nominally should be a galaxy composed of old stars.
		The recessional velocity of NGC 7331 is only 816 km/sec, while the velocities for the other galaxies in the 2MASS mosaic range from 6315 to 8800 km/sec for NGC 7335, 7336, 7337, and 7340 (in increasing eastward distance from NGC 7331).
		Imaging NGC 7814 in the near-IR with 2MASS allows a satisfactory decomposition of the bulge and disk in the galaxy and the determination of the fundamental characteristics of both components (Peletier & Knapen 1992, Messenger, 70, 57).
	www.ipac.caltech.edu /2mass/gallery/images_galaxies.html (5729 words)

	Hubble Nebulae
		NGC 7027 is located about 3,000 light-years from Earth in the direction of the summer constellation Cygnus.
		NGC 6369 lies in the direction of the constellation Ophiuchus, at a distance estimated to be between about 2,000 and 5,000 light-years from Earth.
		The Hubble photograph of NGC 6369, captured with the Wide Field Planetary Camera 2 (WFPC2) in February 2002, reveals remarkable details of the ejection process that are not visible from ground-based telescopes because of the blurring produced by the Earth's atmosphere.
	www.utahskies.org /HST/Archives/nebulae.html (0 words)

	/ftp/cats/J/ApJ/456/174
		J/ApJ/456/174 Intermediate-Mass Population in NGC 604 (Hunter+ 1996) ================================================================================ The intermediate stellar mass population in NGC 604 determined from Hubble Space Telescope Images Hunter D.A., Baum W.A., O'Neil E.J.JR., Lynds R.
		Color- magnitude diagrams of the stars in NGC 604 show a main sequence detected down to an M_F555W,0 of -1 (nearly 6M_sun_).
		The density of the luminous stars in NGC 604 is also comparable to that of OB associations in those galaxies even though the total number of stars is greater in NGC 604.
	vizier.u-strasbg.fr /viz-bin/ftp-index?/ftp/cats/J/ApJ/456/174 (310 words)

	Разноцветная туманность NGC 604 - место рождения новых звезд в ...
		Туманность NGC 604 является самой крупной областью рождения новых звезд в галактике M33, а среди туманностей Местной группы галактик по количеству молодых звезд ее обгоняет только туманность Тарантула из Большого Магелланова облака.
		В туманности NGC 604 астрономы насчитали более 200 очень ярких голубых звезд, которые находятся в облаке светящихся газов размером около 1300 световых лет в поперечнике.
		Яркие звезды в NGC 604 очень молоды - им всего около 3 млн лет.
	news.cosmoport.com /2003/12/08/8.htm (246 words)

	Hubble Heritage: Ein Feuerwerk von Sternentstehung
		Die untersuchte Region trägt den Namen NGC 604 und gehört mit zu den größten Sternentstehungs-Regionen in unserer galaktischen Nachbarschaft.
		NGC 604 liegt in einem Spiralarm der Galaxie M33, die ungefähr 2,7 Millionen Lichtjahre von der Erde entfernt liegt.
		NGC 604 ist für die Astronomen auch deswegen interessant, weil es sich bei dem Nebel um eine lokale Miniaturausgabe einer so genannten Starburst-Galaxie handelt, in der mit einer enormen Rate neue Sterne entstehen.
	www.astronews.com /news/artikel/2003/12/0312-005.shtml (393 words)

	M33 (Site not responding. Last check: 2007-10-29)
		Also because of the cataloging of Herschel, the brightest and largest HII region (diffuse emission nebula containing ionized hydrogen) has obtained a NGC number of its own: NGC 604 (William Herschel's H III.150); it is situated in the northeastern part of the galaxy.
		This is one of the largest H II regions known at all: it has a diameter of nearly 1500 light years, and a spectrum similar to the Orion nebula M42.
		The giant emission nebula NGC 595 was investigated by William H. Waller with the HST (e.g.
	www.intercom.net /user/shaffer/messier/m33.html (810 words)

	Imágenes Celestes: NGC 604, guardería estelar en el Triángulo (Site not responding. Last check: 2007-10-29)
		NGC 604 es similar a las guarderías estelares conocidas en nuestra Vía Láctea tales como la Nebulosa de Orión, pero es mucho mayor en extensión y contiene estrellas formadas mucho más recientemente.
		NGC 604 se encuentra en un brazo espiral de la cercana galaxia M33, localizada a unos 2,7 millones de años luz (830 kiloparsecs) en la dirección de la constelación del Triángulo.
		NGC 604 proporciona a los astrónomos del Hubble un ejemplo cercano de una guardería estelar gigante.
	www.astroseti.org /vernew.php?codigo=1209 (879 words)

	Zwicky 18 - pod galaxy may be orphan from bigger (Site not responding. Last check: 2007-10-29)
		Spiral galaxy Ngc 6118 in an Eso release is larger when dim media contents in the photo are enhanced, the growth in supersize seen at either end where diffuse matter and loosely bonded arms materials are seen extending the galaxy's overall cross section diameter.
		The boil off the core end of Ngc 7424 may help explain a vaguely seen circular in a highly enhanced image by Hubble of Ngc 1808, by professional astronomer James Flood whose interest was in certain spectrum frequencies and wavelengths the galaxy.
		As shown in the next 3d stereo pair, there is a formation which has a circular edge, long steady view in 3d suggests at least one of the boils (the lower of the two) is fractal with six sided geometry edges and for this reason the image is featured in the tympani resonator page.
	www.cosmicastronomy.com /public_html/zwicky.htm (1797 words)

	NGC2403text
		NGC 2403 is a luminous member of the M81 group of galaxies.
		Similar in morphology to M33, NGC 2403 is noted for its exceptionally bright HII regions and high rate of star formation.
		In a recent survey NGC 2403 was found to possess at least six of these monster clouds, an unusually high number for a galaxy.
	www.robgendlerastropics.com /NGC2403text.html (0 words)

	Nebula NGC 604
		Nebula NGC 604 is an enormous cloud of stars, gas, and dust some three million light years away in the nearby spiral galaxy M33 toward the constellation Triangulum.
		The green glow of the nebula is produced by Oxygen ions powered by ultraviolet light from more than 200 bright, hot stars, which are visible as the pink objects concentrated toward the center of the image.
		Gaseous nebulae like NGC 604 are usually found in the arms of spiral galaxies, where they provide the raw material from which new stars are formed.
	www.astrographics.com /GalleryPrintsIndex/GP0020.html (0 words)

	Firestorm of Star Birth Seen in a Local Galaxy
		This festively colorful nebula, called NGC 604, is one of thelargest known seething cauldrons of star birth in a nearbygalaxy.
		NGC 604 is similar to familiar star-birth regions inour Milky Way galaxy, such as the Orion Nebula, but it is vastlylarger in extent and contains many more recently formed stars.
		Thebright stars in NGC 604 are extremely young by astronomicalstandards, having formed a mere 3 million years ago.
	www.spacetelescope.org /images/html/opo0330a.html (148 words)

	Outer parts of M33
		However, despite its low surface brightness, this galaxy was among the first to be identified as a 'spiral nebula' by Lord Rosse in the 1840s.
		In the upper left (north-east) part of this wide field view is the reddish nebula NGC 604, one of the biggest and most active nearby starforming regions.
		NGC 598 Gx 01 33.9 +30 39 s Tri 62.
	www.aao.gov.au /AAO/images/captions/int006.html (210 words)

	NGC 604: Giant Stellar Nursery in M33 - Astronomy News - Care2.com
		NGC 604: Giant Stellar Nursery in M33 - Astronomy News - Care2.com
		To reply to it you must re-activate it.
		Explanation: The nebula cataloged as NGC 604 is a giant star forming region, 1500 light years across, in the nearby spiral galaxy, M33.
	www.care2.com /c2c/groups/disc.html?gpp=9395&pst=971475 (174 words)

	wetteb.de - NGC_604
		NGC 604 ist ein Gasnebel in der Galaxie M33 im Sternbild Dreieck.
		NGC 604 hat eine Winkelausdehnung von 2' × 2' und wurde am 11.
		NGC 604 gehört zu den größten bekannten Gasnebeln.
	www.wetteb.de /wiki_NGC_604 (208 words)

	Non-Messier NGC, IC, and other objects in this database (Site not responding. Last check: 2007-10-29)
		NGC 2547, Lacaille III.2, considerable cluster in Vela
		NGC 3766, Lacaille III.7, considerable southern cluster in Centaurus
		NGC 4833, southern globular in Musca, Lacaille I.4
	astronomy.nju.edu.cn /astron/Messier/ngc.html (676 words)

	Rosa M. González Delgado: publications in refereed international journals.
		Ultraviolet-Optical Observations of the Seyfert 2 galaxies NGC 7130, NGC 5135 and IC 3639: Implications for the Starburst-AGN Connection.
		The circumnuclear region in the Seyfert 1 galaxy NGC 3227.
		The circumnuclear region in the Seyfert 2 galaxy NGC 5953.
	www.iaa.es /~rosa/publicaciones.html (868 words)

	Taringa! - El Universo en Fotos
		Las luminosas estrellas de NGC 604 son extremadamente jóvenes, ya que se han formado hace tres millones de años.
		NGC 4603 se encuentra a 108 millones de años luz, en el cúmulo de galaxias de Centaurus, uno de los más masivos.
		NGC 1569 es una galaxia enana irregular situada a 7 millones de años-luz hacia la constelación de Camelopardalis.
	www.taringa.net /posts/imagenes/802083/El-Universo-en-Fotos.html (8023 words)

	Nebulae
		NGC 2174 01/05/00 LRGB each 4x10 min FS102
		NGC 2244 12/29/99 LRGB each 6x10 min FS102
		NGC 2261 Hubble's Variable Nebula 3x10 16" RC NGC 2264 Cone Nebula 03/25/00 L 6x10 RGB 4x10 2x2 16" RC NGC 2392 02/09/00 RGB 3x10min each 16"RC NGC 3242 (Ghost of Jupiter) 4/9/00 LRGB 3x10 2x2
	www.astroimager.com /nebulae.htm (0 words)

	APOD: 2002 November 2 - NGC 604: Giant Stellar Nursery
		Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer.
		Explanation: Scattered within this cavernous nebula, cataloged as NGC 604, are over 200 newly formed hot, massive, stars.
		At 1,500 light-years across, this expansive cloud of interstellar gas and dust is effectively a giant stellar nursery located some three million light-years distant in the spiral galaxy, M33.
	antwrp.gsfc.nasa.gov /apod/ap021102.html (0 words)

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