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	NGC 2403 - Galaxy in Camelopardalis
		One of these galaxies is NGC 2403, the showpiece of Camelopardalis.
		It is a large, loose-structured spiral galaxy lying in the constellation's southeast corner.
		NGC 2403 can be seen easily as a large hazy spot in binoculars, and a telescope will show a bright elliptical haze surrounded by a faint outer halo.
	www.nightskyinfo.com /archive/ngc2403_galaxy (172 words)

	NGC 2403, Spiral Galaxy
		NGC 2403 in Camelopardalis is a relatively close and bright Spiral Galaxy with a small dim nucleus and open spiral arms.
		NGC 2403 was the first galaxy beyond the Local Group in which Cepheid variables were found.
		NGC 2402 was the host of two observed supernovae before the discovery of SN 2004dj.
	www.kopernik.org /images/archive/n2403.htm (250 words)

	The M81 Group
		NGC 2403 is another prominant spiral galaxy on the right side of the group.
		NGC 2403 (centre) is the second largest galaxy in the M81 group.
		NGC 4236 (right) is a large galaxy in the left side of the M81 group.
	www.atlasoftheuniverse.com /galgrps/m81.html (607 words)

	Universe Today - Spiral Galaxy NGC 2403
		NGC 2403 is an Sc type galaxy with open spiral arms and a small nucleus.
		At a distance of 10 million light years, NGC 2403 is an Sc type galaxy, which has open spiral arms and a small nucleus.
		NGC 2403 has become an important standard galaxy when deciding the distances to other galaxies, as we recognize the vast expanse of space.
	www.universetoday.com /am/publish/spiral_galaxy_ngc2403.html (377 words)

	APOD: 2006 July 5 - Spiral Galaxy NGC 2403 from Subaru (Site not responding. Last check: 2007-10-17)
		NGC 2403 is located just beyond the Local Group of Galaxies, at a relatively close 10 million light years away toward the
		NGC 2403 has a designated Hubble type of Sc.
		In 2004, NGC 2403 was home to one of the brightest supernovas of modern times.
	antwrp.gsfc.nasa.gov /apod/ap060705.html (156 words)

	GIC - Bodes galaxy cluster - big swirls in deep space (Site not responding. Last check: 2007-10-17)
		Galaxy Ngc 2403 is cited as being within the local Bodes (M81) group although few images of Ngc 2403 were found (here is one poor quality from SEDS) searching the Internet.
		The enhancement (by histogram equalize) reveals an Ngc 2403 galaxy superstructure which is much larger than the galaxy structure seen in normal ranges of optical brightness.
		A colored Ngc 2403 original from this site inspects the core, which is very irregular with no core bubble otherwise generated as a long time stable figure.
	www.cosmicastronomy.com /public_html/bodes4.htm (1592 words)

	NGC2403text (Site not responding. Last check: 2007-10-17)
		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 (254 words)

	NGC 2403 - Wikipedia, the free encyclopedia
		NGC 2403 is an intermediate spiral galaxy in the Camelopardalis constellation.
		The northern spiral arm connects to NGC 2404.
		Allan Sandage detected Cepheid variables in NGC 2403 using the Hale telescope, making it the first galaxy beyond our local group to have Cepheids found in it.
	en.wikipedia.org /wiki/NGC_2403 (149 words)

	NRAO Image Gallery
		NGC 2403 is a well-known spiral galaxy in the northern sky.
		Galaxies such as NGC 2403 contain, apart from billions of stars that are visible in the right image, a large disk of hydrogen gas.
		The image on the left shows, on the same scale as the optical image, the hydrogen disk of NGC 2403 as observed with the VLA C array.
	www.nrao.edu /imagegallery/php/level3.php?id=510 (220 words)

	Grupo M81
		NGC 2403 é uma outra galáxia espiral proeminente, no lado direito do grupo.
		NGC 2366 (esquerda) é uma galáxia irregular onde recentemente ocorreram formações de estrelas.
		NGC 2976 (esquerda) é uma pequena galáxia espiral, aproximadamente dois milhões de anos-luz atrás de M81.
	atlas.zevallos.com.br /m81.html (587 words)

	Ole's Astronomy Site: M81 Galaxy Group (Site not responding. Last check: 2007-10-17)
		The M81 Galaxy Group is located at a distance of 12 million light years and comprises about 30 galaxies including the three bright galaxies M81, M82 and NGC 2403.
		NGC 3077 (magnitude 9.9) is the galaxy to the lower left and is often overlooked when observing the two brighter galaxies
		A bright supernova (the brightest since 1993!) appeared in NGC 2403 in July 2004.
	www.ngc7000.org /ccd/gal-m81.html (222 words)

	Universe Today - Supernova in Nearby Galaxy NGC 2403
		The large number of massive stars in NGC 2403 leads to a high supernova rate.
		The heart of NGC 2403 is the glowing region at lower left.
		The myriad of faint stars visible in the Hubble image belong to NGC 2403, but the handful of very bright stars in the image belong to our own Milky Way Galaxy and are only a few hundred to a few thousand light-years away.
	www.universetoday.com /am/publish/supernova_ngc_2403.html?292004 (639 words)

	HubbleSite - NewsCenter - A Bright Supernova in the Nearby Galaxy NGC 2403 (09/02/2004) - Release Images (Site not responding. Last check: 2007-10-17)
		Its home is in the outskirts of NGC 2403, a galaxy located 11 million light-years from Earth.
		The heart of NGC 2403 is the glowing region at lower left.
		The myriad of faint stars visible in the Hubble image belong to NGC 2403, but the handful of very bright stars in the image belong to our own Milky Way Galaxy and are only a few hundred to a few thousand light-years away.
	hubblesite.org /newscenter/newsdesk/archive/releases/2004/23/image/a (650 words)

	NGC 2403 mit Supernova SN 2004dj (Site not responding. Last check: 2007-10-17)
		NGC 2403 Gx 07h 36,9m +55° 36' 8m5 25.5'x13.0' Cam
		Der Kern der Galaxie ist schwach zu erkennen, aber unter den Bedingungen ist nichts von Struktur zu erkennen.
		NGC 2403: Observation of the supernova 2004dj in the bright sky of with a nearly full moon and in lower culmination.
	www.schoenball.de /astronomie/zeichnungen/ngc2403sn2004dj.htm (131 words)

	NGC 2403
		This beautiful spiral galaxy is an outlying member of the M81 group of galaxies, and thus about 12 million light years distant.
		NGC 2403 is among the more conspicuous Northern objects which Charles Messier missed when compiling his catalog.
		This supernova was situated 36E, 100N of the galaxy's nucleus and reached mag 16.0 in its maximum.
	www.seds.org /messier/xtra/ngc/n2403.html (145 words)

	Caltech Astronomy : Palomar Observatory spiral galaxy NGC 2403
		Caltech Astronomy : Palomar Observatory spiral galaxy NGC 2403
		The spiral galaxy known as NGC 2403 is a member of the M81 group of galaxies.
		Instead he may have seen the outburst of a very massive luminous blue variable star located within NGC 2403.
	www.astro.caltech.edu /palomar/ngc2403.html (247 words)

	NGC 2403 - bedeutung definition erklärung glossar zu NGC 2403 (Site not responding. Last check: 2007-10-17)
		NGC 2403 - bedeutung definition erklärung glossar zu NGC 2403
		NGC 2403 ist die Bezeichnung einer Galaxie im Sternbild Giraffe.
		NGC 2403 hat eine Winkelausdehnung von 23.4'x 11.8' und eine scheinbare Helligkeit von +8,50 mag.
	ngc_2403.lexikona.de /art/NGC_2403.html (79 words)

	Ole's Astronomy Site - Supernovae
		Last year I made this image of NGC 2403.
		NGC 6207 is located next to the famous globular M13.
		SN 2003hl and 2003iq in NGC 772 (Aries)
	www.ngc7000.org /ccd/supernova.html (1035 words)

	NGC 2403 (Site not responding. Last check: 2007-10-17)
		NGC 2403 is a spiral galaxy of the Hubble type Sc, meaning it has well-evolved spiral arms and a small central core component.
		In fact, it is still little-known today, maybe because of its isolated location in Camelopardalis, the giraffe, a very inconspicuous constellation, which is, however, circumpolar for mid-northern latitudes.
		NGC 2403 is known to be an outlying member of the M81 group of galaxies, and thus about 10-12 million light years distant.
	astro.nightsky.at /Photo/Gal/NGC2403_Newton.html (175 words)

	[21.04D] Distances to M101, NGC 2403, and NGC 2366 via Long Period Variables (Site not responding. Last check: 2007-10-17)
		To verify the effectiveness of these RSV PL relations, the distances to the galaxies M101, NGC 2403, and NGC 2366 were determined.
		The number of RSVs discovered in M101, NGC 2403, and NGC 2366 was 42, 61, and 20, respectively.
		By assuming a distance modulus for the Large Magellanic Cloud of 18.5 ±0.1 mag, single epoch I-band photometry of the RSVs was used to construct random phase PL relations resulting in distance moduli for M101, NGC 2403, and NGC 2366 of 29.40 ±0.16, 27.67 ± 0.16, and 27.86 ±0.20 mag, respectively.
	www.aas.org /publications/baas/v30n4/aas193/212.htm (371 words)

	DSS Images for NGC 2400 thru NGC 2499
		All of the research images referenced below were generated from the Digitized Sky Survey (DSS), and are covered by this copyright summary and acknowledgement.
		First generation research images were generated from the 102 disk CD-ROM version of the DSS, and second generation DSS research images were generated from the web sites located at The Space Telescope Science Institute, and / or The European Southern Observatory.
		Identification of objects, in the vicinity of the featured NGC object, was accomplished through the use of NASA's Extragalactic Database (NED) with this acknowledgement.
	www.ngcic.org /dss/dss_n2400.asp (300 words)

	Supernova 2004dj in NGC 2403 (Site not responding. Last check: 2007-10-17)
		Following previous work [3], we assume that the empirical relation between the equivalent width of Na I D1 and interstellar reddening in our Galaxy [4] is also representative for the interstellar medium in NGC 2403.
		H-alpha image of NGC 2403 obtained with the Tautenburg Schmidt focus CCD camera in 2003.
		H-alpha image of NGC 2403 obtained with the Tautenburg Schmidt focus CCD camera on August 10, 2004 by B. Stecklum.
	www.tls-tautenburg.de /research/klose/SN2004dj.html (441 words)

	APOD: 2004 September 7 - A Supernova in Nearby Galaxy NGC 2403 (Site not responding. Last check: 2007-10-17)
		APOD: 2004 September 7 - A Supernova in Nearby Galaxy NGC 2403
		Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer.
		recorded just over a month ago in the outskirts of nearby galaxy NGC 2403.
	antwrp.gsfc.nasa.gov /apod/ap040907.html (159 words)

	wpo-supernovae SN2004dj [NGC 2403] + SN2004et [NGC 6946] (Site not responding. Last check: 2007-10-17)
		SN2004dj in NGC 2403 [Cam] + SN2004et in NGC 6946 [Cyg]
		The supernova is near the NE edge of NGC 2403 and well placed for visual and CCD observations.
		The discovery was made on July 31.76 at roughly V magnitude of 11.2 and confirmed on Aug. 1.45 at V=11.3.
	home.freeuk.com /m.gavin/2004dj.htm (323 words)

	NGC 2403 (Site not responding. Last check: 2007-10-17)
		NGC 2403 is a fine spiral galaxy ten million light years away.
		Having verified that you're in the right location, now put 42 and 43 at the northwest corner of your field of vision.
		NGC 2403 is at the opposite side: binoculars.
	www.dibonsmith.com /ngc2403.htm (104 words)

	NGC2403
		NGC 2403 is an outlying member of the M81 group.
		This galaxy has a suprisingly low surface brightness.
		These hydrogen clouds are regions of potential future star formation.
	www.dsi-astronomie.de /NGC2403.htm (88 words)

	Galaxy NGC 2403 and supernova 2004dj
		NGC 2403 was difficult to see because of bright background sky.
		West spiral arm is quite massive and bright.
		NGC 2404 is a lonely patch near by SN200dj which is about 12 mag.)
	kotisivu.mtv3.fi /deepsky/havaintongc2403.htm (82 words)

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