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Topic: Elliptical Galaxy M110

	Encyclopedia: Elliptical Galaxy M110 (Site not responding. Last check: 2007-11-04)
		The Elliptical Galaxy M110 (also known as Messier Object 110, Messier 110, M110, or NGC 205) is an elliptical galaxy in the Andromeda constellation, a satellite of the Andromeda Galaxy, and a member of the Local Group galaxies.
		Herschel 18-5 - NGC 205 / M110 (Elliptical Galaxy)
		Herschel 18-5 / NGC 205 / M110 - Elliptical Galaxy
	www.nationmaster.com /encyclopedia/Elliptical-Galaxy-M110 (704 words)

	Elliptical galaxy - Wikipedia, the free encyclopedia
		The giant elliptical galaxy NGC 4881 (the spherical glow at upper left) lies at the edge of the Coma Cluster of Galaxies.
		This traditional portrait of elliptical galaxies paints them as galaxies where the star formation was over after the initial burst, now shining only with their aging stars.
		The smallest, the Dwarf elliptical galaxies, may be no larger than a typical globular cluster, but contain a considerable amount of dark matter not present in clusters.
	www.wikipedia.org /wiki/Elliptical_galaxy (432 words)

	Elliptical galaxy - Wikipedia, the free encyclopedia
		Larger elliptical galaxies typically have a system of globular clusters, indicating an old population.
		The Hubble classification of elliptical galaxies ranges from E0 for those that are most spherical, to E7, which are long and thin.
		Elliptical galaxies tend to lie in the cores of galaxy clusters and in compact groups of galaxies.
	en.wikipedia.org /wiki/Elliptical_galaxy (432 words)

	Encyclopedia: Elliptical galaxy (Site not responding. Last check: 2007-11-04)
		Elliptical Galaxy M32 (also known as Messier Object 32, Messier 32, M32, or NGC 221) is a dwarf elliptical galaxy in the Andromeda constellation, a satellite of the Andromeda Galaxy, and a member of the Local Group galaxies.
		Elliptical Galaxy M59 (also known as Messier Object 59, Messier 59, M59, or NGC 4621) is an elliptical galaxy in the constellation Virgo.
		The Spindle Galaxy (NGC 5866), a lenticular galaxy in the Draco constellation.
	www.nationmaster.com /encyclopedia/Elliptical-galaxy (1657 words)

	* Elliptical Galaxy - (Astronomy): Definition (Site not responding. Last check: 2007-11-04)
		Elliptical galaxies are characterised by an absence of spiral arms.
		Elliptical galaxies are comprised mostly of old stars and contain very little dust and "cool" gas that can form stars.
		Observations of the core of the elliptical galaxy M87 showed a source that was blueshifted on one side and redshifted on the other, spinning so fast that the central object had to be compact and enormous.
	www.bestknows.com /astronomy/elliptical_galaxy.html (1144 words)

	Hubble sequence : Elliptical galaxy (Site not responding. Last check: 2007-11-04)
		Elliptical galaxies are generally fairly low in gas and dust, and are composed mostly of older stars.
		Spiral galaxies generally have plentiful supplies of gas and dust, and have a broad mix of older and younger stars.
		From this, astronomers have constructed a theory of galaxy evolution which suggests that ellipticals are, in fact, the result of collisions between spiral and/or irregular galaxies, which strip out much of the gas and dust and randomize the orbits of the stars.
	www.termsdefined.net /el/elliptical-galaxy.html (446 words)

	ipedia.com: Local Group Article (Site not responding. Last check: 2007-11-04)
		NGC 1569 - Irregular Galaxy (Irp+ III-IV) in Camelopardalis
		Camelopardalis A - Irregular Galaxy (Irr) in Camelopardalis
		UGC 9128 (DDO 187) - Irregular Galaxy (Irp+) in Boötes
	www.ipedia.com /local_group.html (649 words)

	Elliptical Galaxies (Site not responding. Last check: 2007-11-04)
		Elliptical galaxies constitute approximately 10% of observed galaxies.
		Some other examples of elliptical galaxies include M32, which is an E2 dwarf elliptical near the Andromeda Galaxy, and the E6 elliptical galaxy M110, another satellite of the Andromeda Galaxy.
		Elliptical galaxies exhibit far less evidence for young stars, gas, or dust than do spiral galaxies, and have larger random motion of stars than in spiral galaxies where the motion is a more ordered rotation.
	csep10.phys.utk.edu /astr162/lect/galaxies/elliptical.html (257 words)

	M110 Galaxy in Andromeda (Site not responding. Last check: 2007-11-04)
		M110 is a satellite galaxy of the great Andromeda Galaxy.
		M110 is a large bright E5 elliptical galaxy.
		M110 is the galaxy in the lower right portion of the image.
	members.cox.net /sidleach/m110.htm (250 words)

	Messier Object 110
		Independent of Messier's discovery, Caroline Herschel discovered M110 on August 27, 1783, little more than 10 years after Messier, and William Herschel numbered it H V.18 when he cataloged it on October 5, 1784.
		The small elliptical galaxy M110 is at about the same distance as the Andromeda galaxy M31, about 2.9 million light years, as confirmed by Walter Baade in 1944, when he resolved it into stars (Baade 1944).
		However, as it is much brighter than typical dwarf spheroids, Sidney van dan Bergh has recently introduced the term "Spheroidal Galaxy" for this and similar galaxies, including Local Group members NGC 147 and NGC 185.
	www.seds.org /messier/m/m110.html (311 words)

	Cosmic Voyage-The Online Resource for Amateur Astronomers (Site not responding. Last check: 2007-11-04)
		M32 is a magnitude 8.0 elliptical galaxy, 4' in diameter, with a bright core.
		M110 is seen just inside the northern edge of the field.
		This elliptical galaxy covers a 15'x6' area and is the most difficult of the three to detect.
	hometown.aol.com /billferris/m31.html (368 words)

	Galaxies (Site not responding. Last check: 2007-11-04)
		Statistical arguments suggest that the distribution of galaxies among the ellipticities is roughly uniform.
		For some reason Elliptical galaxies formed all their stars a long time ago, using up all their gas, so that new stars are no longer forming, there is virtually no young stellar population nor gas nor dust.
		It seems almost certain, for example, that the giant elliptical galaxies seen at the centers of rich clusters formed as galaxies gradually accumulated at the center of the cluster's strong gravitational field.
	cassfos02.ucsd.edu /public/tutorial/Galaxies.html (1087 words)

	Hubble sequence - Psychology Central
		An elliptical galaxy (E0-7) has an ellipsoidal form, with a fairly even distribution of stars throughout.
		A lenticular galaxy (S0 and SB0) appears to have a disk-like structure with a central spherical bulge projecting from it, and does not show any spiral structure.
		A barred spiral galaxy (SBa-d) has a similar sort of spiral structure to spiral galaxies, but instead of emanating from the bulge, the arms project out from the ends of a "bar" running through the bulge, like ribbons on either end of a baton.
	psychcentral.com /psypsych/Hubble_sequence (457 words)

	APOD Search Results for "elliptical galaxy"
		galaxies of the Hercules Cluster, an archipelago of
		Galaxy M87 is about 50 million light-years away and reigns as the large central elliptical galaxy in the Virgo cluster.
		Elliptical galaxies are ellipsoidal in shape, contain no spiral arms, contain little interstellar gas or dust, and are found mostly in rich clusters of galaxies.
	antwrp.gsfc.nasa.gov /cgi-bin/apod/apod_search?elliptical%2Bgalaxy (10745 words)

	Elliptical Galaxy
		Elliptical galaxies are spheroidal distributions of mostly older stars, usually without much of the...
		Elliptical Galaxy UGC 9799 - Galaxy Cluster Abell 2052...
		In general, then, an elliptical galaxy is given the label En, where the number n is determined by...
	www.elliptical-exercise.com /elliptical-exercise-3/elliptical-galaxy.html (782 words)

	ELLIPTICAL GALAXY FACTS AND INFORMATION
		The single largest known galaxy, M87 (which also goes by the NGC number 4881), is an elliptical.
		Current thinking is that an elliptical galaxy is the result of a long process where one or more smaller galaxies, of any type, collide and fuse in a larger one.
		This fusion process may at time carry on until recent or contemporary ages, and is not limited to giant elliptical.
	www.abait.com /elliptical_galaxy (355 words)

	Messier Object 110 (Site not responding. Last check: 2007-11-04)
		M110 is the second brighter satellite galaxy of the Andromeda galaxy M31, together with M32.
		Independent of Messier's discovery, Caroline Herschel discovered M110 on August 27, 1783, little more than 10 years after Messier, and William Herschel numbered it 18 H V. The small elliptical galaxy M110 is at about the same distance as the Andromeda galaxy M31, about 2.2 million light years.
		Apparently, this dwarf elliptical galaxy has also several globular clusters in a halo around it.
	astroa.physics.metu.edu.tr /messier/m/m110.html (176 words)

	Superform of Andromeda is vast (Site not responding. Last check: 2007-11-04)
		The Andromeda superform is not inconsistent with a partial elliptical galaxy such as the Sombrero (3d-somb1.htm, 3d-sombr.htm, sombre-2.htm) whose halo is shallow and diffuse and tilted (lower foreground slanting through the middle to upper half canted rearward) with a strong central disk which is thin and spread out in a wide cross sectional area.
		The Hunter image contains a large value object near and to the left of M110, the object is nearly the size of M110 and may be a dwarf galaxy farther back in deep space obscured by foreground dust and haze.
		M110 is a difficult galaxy for photographers in having an undistinguished center so small it's pin point size is hardly bigger than a cluster of newbirn ultra hot supergiant stars.
	www.cosmicastronomy.com /hunter.htm (1700 words)

	Elliptical Galaxies (Site not responding. Last check: 2007-11-04)
		Elliptical galaxies are ellipsoidal agglomerations of stars, which usually do not contain much interstellar matter, and look smoothly like small wads in the telescope.
		lenticulars, can hardly be distinguished from (and thus are sometimes misclassified as) elliptical galaxies; this has happened in the past to all four Messier lenticulars, among many others.
		Structure and Dynamics of Elliptical Galaxies, by Tim de Zeeuw and Marijn Franx, Annual Review of Astronomy and Astrophysics 1991, 29:239-274.
	www.seds.org /messier/elli.html (157 words)

	Autumn Telescopic Wonders
		M31, M32 and M110 Better known as the Andromeda Galaxy and its companion galaxies, the view is made to order for the smaller telescope.
		The galaxy is larger than out own and lies at a distance of a bit more than 2 million light years.
		The nearly spherical M32 is seen nearby, while the faint elliptical galaxy M110 is barely visible on the other side of M31.
	ourworld.compuserve.com /homepages/bmoler/autumn.htm (815 words)

	Messier Object 110 (Site not responding. Last check: 2007-11-04)
		The small elliptical galaxy M110 is at about the same distance as the Andromeda galaxy M31, about 2.9 million light years.
		It is of type E5 or E6 and is designated "peculiar" because it shows some unusual dark structure (probably dust clouds); it is now often classified as a dwarf spheroid galaxy, not a generic elliptical one (this would make it the first ever known dwarf spheroid, of course).
		Its mass was estimated to be between 3.6 and 15 billion solar masses.
	digilander.libero.it /COA/m110.htm (229 words)

	M32: Elliptical Galaxy
		M32 is a satellite galaxy to the famous naked eye spiral galaxy, M31, in Andromeda.
		It was discovered by le Gentil in 1749, the first elliptical galaxy ever seen, and was catalogued by Charles Messier in 1764.
		There are several close companion galaxies, the most prominent are M31 (NGC224) and M110 (NGC205).
	www.r-clarke.org.uk /messier/m32.htm (89 words)

	NOAO Image Gallery: Elliptical Galaxies
		Elliptical galaxies are spheroidal distributions of mostly older stars, usually without much of the intersteller material that is prevalent in spirals.
		Ellipticals are often classified with a number that describes their appearance; an E0 galaxy is almost perfectly circular while an E7 is quite elongated.
		Ellipticals vary greatly in size, from very small companions found near our own galaxy to the giant ellipticals often seen near the center of rich clusters.
	www.noao.edu /image_gallery/elliptical_galaxies.html (171 words)

	Messier Year in a Night
		At galaxy central is a faint 12.5 magnitude star-like core.
		Galaxy M105 is smaller than M96 - say a roundish 4 arc-minutes, Its core is quite bright and gives a sense of elongation west-southwest.
		The galaxy is visibly elongated with a sharper edge to the west.
	astro.geekjoy.com /specreps/night_year.html (22671 words)

	Elliptical Galaxy M110 - Encyclopedia, History, Geography and Biography
		Elliptical Galaxy M110 - Encyclopedia, History, Geography and Biography
		This encyclopedia, history, geography and biography article about Elliptical Galaxy M110 contains research on
		Elliptical Galaxy M110, External link, Andromeda constellation, Dwarf elliptical galaxies, Local Group, Andromeda Subgroup, NGC objects and Messier objects.
	www.arikah.net /encyclopedia/NGC_205 (124 words)

	Stars Galaxies and Beyond / The Solar System Tour / Meatnpotatoes.com (Site not responding. Last check: 2007-11-04)
		Irregular or Lenticular Galaxy UGCA 92 in Camelopardalis
		Elliptical Galaxy M49 of Virgo Cluster (in Virgo)
		Elliptical Galaxy M59 of Virgo Cluster (in Virgo)
	www.meatnpotatoes.com /solar-beyond.html (1096 words)

	The Local Group
		Messier objects: The Andromeda Galaxy M31 and its satellites M32 and M110, as well as the Triangulum Galaxy M33.
		The next more distant galaxy groups, the NGC 4244 group and the CVn I Cloud (with M94 and M64) are probably too remote to have interacted significantly with the Local Group in the past.
		Galaxies marked with "(I)" are newly taken into the list from Irwin's list: Besides the newly discovered Antlia dwarf, these are the Phoenix dwarf, UGCA 92, Sextans B, and NGC 3109.
	www.seds.org /messier/more/local.html (1596 words)

	m110 (Site not responding. Last check: 2007-11-04)
		M110 is the second brighter satellite galaxy of the
		Andromeda galaxy M31, together with M32, and thus a
		The small elliptical galaxy M110 is at about the same distance as the Andromeda galaxy M31, about 2.2
	nvn-informatika.hr /M100-110/m110.html (198 words)

	Dwarf Elliptical Galaxy NGC 205 in the Local Group
		It is part of a gathering of about 25 galaxies known as the Local Group.
		Pictured on the lower left is one of the many dwarf ellipticals: NGC 205.
		This galaxy is sometimes known as M110, although it was actually not part of
	www.astronet.ru /db/xware/msg/1163939 (209 words)

	Elliptical galaxy M110 (Site not responding. Last check: 2007-11-04)
		The outer immediate companion of the Andromeda galaxy, NGC 205 (sometimes denoted Messier 110).
		Unlike most dwarf elliptical or spheroidal galaxies, it has recognizable dust clouds (two are visible here at about the 7 o'clock and 11 o'clock positions from the nucleus) and clear signs of recent star formation.
		This image shows a 9-arcminute section, seen in red light with Lowell Observatory 1.1m telescope, focal reducer, and TI CCD.
	crux.astr.ua.edu /gifimages/m110r.html (83 words)

	GIC - Stars yield interesting new secrets (Site not responding. Last check: 2007-11-04)
		Suppose, just suppose, this star someday is shielded behind haze, and the popcorn kernal is really there and still crackling at the end of the jet, this could suddenly become very much the look and feel of some of the smaller dark shafted 'eyestalks' under study at this GIC page.
		An elliptical large star, yellow colored, has shown up in a VLT image of giant spiral galaxy Ngc 2997, the star (if it is a star) rended by telescope overplus, and is only partially captured, nonetheless what is seen shows elliptical disks displacing to the upper left around a central slightly irregular orb.
		A Streaker moving around is seen leaving the main body of small galaxy Ngc 4214, leaving a smokey stover in the form of a dragging trail composed of hot blue new stars, seen in high enhancement.
	cosmicastronomy.com /stars.htm (4120 words)

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