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Topic: NGC 206

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	List of NGC objects - Wikipedia, the free encyclopedia
		NGC 317A - a lenticular galaxy in Andromeda
		NGC 429 - a lenticular galaxy in Cetus
		NGC 448 - a lenticular galaxy in Cetus
	en.wikipedia.org /wiki/List_of_NGC_objects (4108 words)

	NGC 206: Starcloud in the Andromeda Galaxy M31 (Site not responding. Last check: 2007-11-03)
		NGC 206: Starcloud in the Andromeda Galaxy M31
		Barbara Mochejska created this color image of the NGC 206 field of M31 from data of the DIRECT project, an attempt to directly determine the distances of the Local Group galaxies M31 and M33, with Cepheid and eclipsinf binary variables.
		Also note Martin Germano's image of the southwestern part of M31, showing M32 and NGC 206, and in particular the higher-res magnification of the NGC 206 and M32 part of this image.
	www.seds.org /messier/more/m031_n206.html (185 words)

	[No title]
		NGC 1113 - 02 50.2 +13 18 r Ari vF NGC 1056 Gx 02 42.9 +28 33 r Ari 13.
		NGC 5804 Gx 14 55.7 +49 39 r Boo vF, vS, vsmbM, 6 nr NGC* 5611 Gx 14 24.2 +33 01 r Boo 13.
		NGC 5922 Gx 15 21.2 +41 40 h Boo 0.5 15.
	www.phonetik.uni-muenchen.de /Mitarbeiter/Kotten/Transport/NGC2000sort.dat (17282 words)

	Visual Observations
		NGC 7009, the Saturn Nebula, was given the designation of H IV-1 as it was the 1st planetary nebula he discovered, while NGC 7662, the Blue Snowball Nebula, was given the designation of H IV-18 as it was the 18th planetary nebula he discovered.
		NGC 206, a starcloud in one of the arms of M31, was visible as well.
		M42 (NGC 1976), The Orion Nebula, is an emission nebula and cluster with a magnitude of 3.7 and is 90.0'x60.0' in size.
	members.leapmail.net /~ericj/recent_obs2.html (4865 words)

	HI, Molecules and Dust. (Site not responding. Last check: 2007-11-03)
		Rotating CO rings appear to be present in the nuclei of galaxies NGC1808, NGC 4414, NGC 4565, NGC 4631 and NGC 4945.
		IRAM 30-m antenna observations of edge-on galaxy NGC 4565 reveal 1.2-mm continuum emission (from dust) that follows CO near the nucleus and HI at the periphery; the results are interpreted as the first unambiguous detection of dust emission in extragalactic HI clouds.
		It was found that the CO luminosities and 1.3-mm fluxes correlate, that the emission is concentrated towards the nucleus of starburst galaxies but extended along the spiral disk of non-active galaxies, and that the ratio of total IR luminosity to gas mass is about twenty times higher for active galaxies.
	www.ira.cnr.it /IAU_Com40/c40rpt97/node55.html (1193 words)

	Photo Index (Site not responding. Last check: 2007-11-03)
		NGC 772 and 770 Spiral Galaxy in Aries
		NGC 2486 and NGC 2487 Spiral Galaxies in Gemini
		NGC 5921 Spiral Galaxy in Serpens + SN2001X
	schmidling.netfirms.com /phoindex.htm (332 words)

	Delmarva Stargazers Observing Notes page 5
		NGC 436 is a tight group of rich and bright stars.
		NGC 7082 is also large with a lot of stars.
		NGC 7067 in contrast is a tiny and faint cluster with most of its members in a tight ball.
	www.delmarvastargazers.org /observingnotes/page5.html (868 words)

	Views of ANDROMEDA
		NGC 206 is pretty faint, pretty small, elongated 2X1 in PA0, not brighter in the middle and very mottled.
		NGC 389 Very faint, pretty small, round, not brighter in the middle, there is a 12th mag star 1' NE, averted vision helps with object at 165X.
		NGC 785 This is the other center to Abell 262, there is an edge on very close to NGC 785 and two other faint galaxies nearby.
	www.saguaroastro.org /content/obsnotes/ANDROMEDA.htm (1515 words)

	Deep sky objects in Andromeda
		With your finder scope centred on Gamma Andromedae, move your telescope to the east in the direction of M34 until the double star is almost on the western edge of the field of view of your finder scope.
		NGC 752 is the ball, which lies in front of it.
		But it wasn't a smudge; it was NGC 404 in its full glory, at least 4’ in diameter, with direct vision, and the yellowish Mirach in the same field of view.
	www.backyard-astro.com /focusonarchive/andromeda/andromeda.html (1660 words)

	Hunting the wild pony and other adventures
		NGC 6369 in Ophiuchus, the beautuful mag 11.4 (or is it 14.7) Little Ghost nebula was among my favorite finds as was, NGC 6440 in Sagittarius, a nice round mag 9.7 cluster and 20 arcminutes to the north, NGC 6445, the mag 11.2 Little Gem Nebula.
		NGC 891 is a rich beauty with the dust lane bisecting its edge-on middle.
		NGC 2024, the Flame nebula with its dark lane bisecting the firey brightness was a warm-up project.
	observers.org /reports/98.09.20.html (1440 words)

	APOD: April 2, 1999 - Stars of NGC 206 (Site not responding. Last check: 2007-11-03)
		spiral galaxy Andromeda (M31), the star cluster NGC 206 is one of the largest star forming regions known in our local group of galaxies.
		of NGC 206 betray its youth - but close, systematic studies of variable
		About 3 million light-years away, an accurately known distance to NGC 206 and thus M31 is critical to the larger understanding of galaxy formation, galaxy evolution, and ultimately
	antwrp.gsfc.nasa.gov /apod/ap990402.html (156 words)

	APOD Search Results for "M31" (Site not responding. Last check: 2007-11-03)
		NGC 520, at visual magnitude 12, has been noted to be one of the brightest interacting galaxies on the sky, after interacting pairs of galaxies known as the Antennae.
		NGC 205 to be unusual for an elliptical galaxy in that it contains at least two dust clouds (at 1 and 4 o'clock - they are visible but hard to spot) and signs of recent star formation.
		Like M32, NGC 205 is a companion to the large M31, and can sometimes be seen to the south of M31's centre in photographs.
	www.star.ucl.ac.uk /cgi-bin/apod/apod_search?M31 (7600 words)

	Mark Wagner; Out From The Shadow - A Night At Henry Coe
		NGC 83 will be among a group of three mag 11.2 stars, all within 2' of the galaxy, and forming a small parallelogram with it.
		The last two objects I found in this field were NGC 94 and 96, sitting close together (5' separation) and N of the line between NGC 83 and the mag 7.5 star to the E. NGC 94 is the closer of the pair to the line, but was a "maybe" with averted vision.
		NGC 206, the bright emission knot containing blue supergiant stars south of the core looked much like a large galaxy, very obvious.
	observers.org /reports/2000.08.26.3.html (1757 words)

	Ephemeris
		Following close behind was the hunt for globulars surrounding M33, the Triangulum or Pinwheel galaxy, and finishing off the serious project work with the ambiguous galaxy companions of NGC 7331 in Pegasus, just a hop away from Stephen's Quintet, some of the brighter objects on our list this session.
		The brightest of these and our first target was NGC 206, 50' southwest of the galactic center.
		NGC 205, the other large companion is also known as M-110.
	www.sjaa.net /eph/9812h.html (756 words)

	Catalogue Selection Page
		VI photometry of new Cepheids in NGC 2541 (Ferrarese+, 1998) (
		VI photometry of new Cepheids in NGC 3198 (Kelson+, 1999) (
		VI photometry of new Cepheids in NGC 3319 (Sakai+, 1999) (
	cdsweb.u-strasbg.fr /viz-bin/VizieR-2?-kw.cat=14970188 (695 words)

	Messier Object 31 (Site not responding. Last check: 2007-11-03)
		NGC 206 in the Andromeda Galaxy (M 31) is the largest and perhaps the most massive region in the Local Group with coherent star formation taking place on a timescale of =~30Myr.
		We find that NGC 206 represents the latest phase of an enhanced level of star formation in the southern region of M 31.
		NGC 206 is located at the intersection of two spiral arms, suggesting that the interaction between the spiral arms is responsible for the enhanced levels of star formation.
	ad.usno.navy.mil /~olling/My_Lit_Dat/M31.html (6801 words)

	Spiral Galaxies
		The image shown adjacent left is of the spiral galaxy ESO 269-57, which is in the southern constellation Centaurus (Ref).
		As already noted in conjunction with the Milky Way, This is in fact why the spiral arms of these galaxies are so prominent: because they are regions of active star formation, there are many hot young blue and blue-white stars there, making the spiral arms extremely visible.
		The adjacent image shows a star-forming region in the spiral arms of the galaxy M31 (Andromeda) called NGC 206 (Ref).
	csep10.phys.utk.edu /astr162/lect/galaxies/spiral.html (544 words)

	APOD Search Results for "binary" (Site not responding. Last check: 2007-11-03)
		An expanded view of the region near the core of NGC 5194 reveals x-rays from a supernova remnant, the debris from a spectacular stellar explosion, first detected by earthbound astronomers in 1994.
		Like other normal elliptical galaxies, NGC 4697 is a spherical ensemble of mainly older, fainter, low mass stars, with little star forming gas and dust compared to spiral galaxies.
		As a result, NGC 253 and other similar starforming galaxies could ultimately develop a single, central, supermassive fl hole, transforming their cores into quasars.
	www.star.ucl.ac.uk /cgi-bin/apod/apod_search?binary (10851 words)

	RASC Calgary Centre - Constellation of the Month
		As mentioned, objects are grouped roughly by brightness, ranging from naked eye brightness to being a struggle with a 16" scope.
		The Messier Objects are all present, as are the 110 Finest NGC objects from the The RASC Observer's Handbook as well as many of the objects on the list of RASC Deep-Sky Challenge Objects.
		Small scopes are defined as those up to 6", big scopes from 8" to 10", and challenge objects are best viewed with scopes of 11" diameter and larger.
	calgary.rasc.ca /constellations (589 words)

	[No title] (Site not responding. Last check: 2007-11-03)
		Astronomy Picture of the Day April 2, 1999 Stars of NGC 206 Credit: B.J. Mochejska (Warsaw University), The DIRECT Project, FLWO, MDM Explanation: Nestled within the dusty arms of the large spiral galaxy Andromeda (M31), the star cluster NGC 206 is one of the largest star forming regions known in our local group of galaxies.
		Astronomers are searching for variable stars in NGC 206, particularly pulsating stars known as Cepheids and eclipsing binary star systems.
		About 3 million light-years away, an accurately known distance to NGC 206 and thus M31 is critical to the larger understanding of galaxy formation, galaxy evolution, and ultimately the distance scale of the Universe.
	www.aip.de /gallery/galaxies/ngc206_direct_big.txt (185 words)

	Pemanent past images (Site not responding. Last check: 2007-11-03)
		NGC 80 is the brightest member of this diverse group of Galaxies in Andromeda.
		NGC 2536 is the small galaxy at the end of the plume of material being pulled from the larger S(c) peculiar galaxy NGC 2535.
		NGC 7538 is within 1.5 degrees of NGC 7635 (the Bubble Nebula) and the bright open cluster M 52, both to the east.
	home.earthlink.net /~mcgermano/oldarchive.html (5684 words)

	Andromeda Galaxy
		Subsequently, the "nebula" was also designated as NGC 224 by John Louis Emil Dreyer (1852-1926) in his New General Catalogue (NGC) of Nebulae and Clusters of Stars, which was first published in 1887 and later supplemented with Index Catalogue (IC) I in 1895 and IC II in 1907.
		The brightest star cloud in Andromeda has its own NGC number, NGC 206.
		One of the largest star-forming regions known in the Local Group of galaxies, Sir William Friedrich Wilhelm Herschel (1738-1822, portrait) noted it in his catalog as H V.36 on his discovery of the diffuse object on October 17, 1786.
	www.solstation.com /x-objects/andromeda.htm (2098 words)

	David's Astronomy - Images 2002-10-02 (S00028)
		NGC 7317 (Mag +14.8), NGC 7318A (Mag +14.6), NGC 7318B (Mag +14.0),
		NGC 7319 (Mag +14.6), NGC 7320 (Mag +13.6), NGC 7320C (Mag +16.6)
		NGC 206 Emission Knot in M31 arms (Andromeda)
	www.richweb.f9.co.uk /astro/images-2002-10-02.htm (254 words)

	Simulations of NGC 206 and its Effects on M31 (Site not responding. Last check: 2007-11-03)
		Simulations of NGC 206 and its Effects on M31
		NGC 206 is a very large density enhancement in the outer disk of the nearby spiral galaxy M31.
		Byrd (1984 fnad.proc 26B) and Byrd, Smith, and Miller (ApJ 286, 62-67) have demonstrated that NGC 206 gravitationally affects M31's disk.
	www.aas.org /publications/baas/v29n5/aas191/abs/S105017.html (99 words)

	[41.23] HST Observations of Massive Young Star Clusters in M31 (Site not responding. Last check: 2007-11-03)
		G38 and G44 are located to the south south-west of the giant OB association NGC 206.
		These clusters may have been formed by the same mechanism that has caused the formation of NGC 206 if the density wave interaction located at NGC 206 has been propagating through the southern half of M31 at ~32 km/s with respect to the stars in the disk for the past 100 Myr.
		This propagation velocity is also consistent with the age distribution of the Cepheid population near NGC 206 (Magnier et al.
	www.aas.org /publications/baas/v32n4/aas197/388.htm (273 words)

	APOD Search Results for "M31"
		Interesting features of NGC 520 include an unfamiliar looking tail of stars at the image bottom and a perhaps more familiar looking band of dust running diagonally across the image center.
		In fact, the cavernous NGC 604 is the brightest star forming region seen here, visible along an arm arcing above and to the right of the galaxy center.
		Like M32, NGC 205 is a companion to the large M31, and can sometimes be seen to the south of M31's center in photographs.
	antwrp.gsfc.nasa.gov /cgi-bin/apod/apod_search?M31 (7060 words)

	Minimum Aperture Catalogue: AQUILA (Site not responding. Last check: 2007-11-03)
		6" 3 NGC* 6756 251 I 2 m 10.6 4' 40 19 08.7 +04 41 st11...
		,vF 11" NGC 6941 254 13.5 20 36.3 -04 38 =galaxy?
		NGC 6929 253/254 SA0+p: 13.4v 0.8'x0.7' 20 33.4 -02 02 PA 95° MCG+0-52-38 (254) SAabp sp 14.2 1.7'x0.5' 20 35.5 -02 46 PA 115° MCG-1-52-8 (299) Sc: sp 14.5 2.1'x0.3' 20 35.5 -06 15 edge-on IC 1327 (254) S0+?
	www.astro.helsinki.fi /~kahanpaa/astro/constell/aql.html (866 words)

	Aperture, Who Needs it? (Site not responding. Last check: 2007-11-03)
		I looked at a few of my favorite open clusters: M11 sparkled, though of course it showed fewer stars than are visible through a larger aperture; NGC 457, which I've always known as the "dragonfly", showed nicely; and with a 25mm Plossl, the Double Cluster in Perseus was gorgeous, with both clusters visible.
		M110 was also easily visible, and I could detect a trace of brightening in the area of the star cloud NGC 206.
		A nearby observer with a 4.5" was looking at M22, low in the southwestern sky, so I pointed there as well, and was rewarded with an excellent view of the globular.
	www.shallowsky.com /observing/deepsky80.html (507 words)

	Jari's Astronomy Site
		Center of integration time is 19:35 UT Minor planet 7 Iris is the upper of the bright pair just left of center.
		NGC 6207 is also visible at upper left.
		Even the 13th magnitude star just to the east of the nebula is visible.
	www.kolumbus.fi /jimenez/photos/astro/rubinar (121 words)

	Binoculars, Wide field views in Winter Skies
		Within the southern arm a bright H II region, NGC 206, is visible in the big binoculars and the rest of the spiral arms sparkle with mottling.
		The Alpha Perseus Group is a large, nearby star cluster that surrounds the brightest star in the constellation of the Hero.
		So the entire Orion Nebula complex, including M42, M43 and several NGC nebulae are in this breathtaking field of view.
	www.saguaroastro.org /content/binoculars.htm (1722 words)

	Southern arm of M31 (Site not responding. Last check: 2007-11-03)
		This picture shows less than half the galaxy but the spiral structure, star clouds and dust lanes are evident.
		In his illustration Hubble points out a Cepheid variable star, a globular cluster, a star cloud and open cluster as typical ingredients of a spiral galaxy.
		NGC 224 Gx 00 42.7 +41 16 s And 178.
	www.aao.gov.au /images/captions/int003.html (264 words)

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