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Topic: NGC 7742

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	New General Catalogue
		The NGC was compiled in the 1880s by Dreyer[?] using observations mostly from William Herschel, and then subsequently expanded with two Index Catalogues (ICs).
		NGC 2346 - a planetary nebula in the Monoceros constellation
		NGC 7742 - a Type 2 Seyfert galaxy in the constellation Pegasus.
	www.ebroadcast.com.au /lookup/encyclopedia/ng/NGC.html (204 words)

	New General Catalogue: Definition and Links by Encyclopedian.com - All about New General Catalogue
		The NGC was compiled in the 1880s by Dreyer[?] using observations mostly from William Herschel, and then subsequently expanded with two Index Catalogues (ICs).
		NGC 2346 - a planetary nebula in the Monoceros constellation
		NGC 4321 - M100, a spiral galaxy in the Virgo cluster
	www.encyclopedian.com /ng/NGC.html (237 words)

	ngc (Site not responding. Last check: 2007-10-28)
		NGC 5866 - A lenticular galaxy in the Draco constellation
		NGC 6121 - M4, a globular cluster in the Scorpius constellation
		NGC 6402 - M14, a globular cluster in the Ophiuchus constellation
	www.yourencyclopedia.net /NGC.html (357 words)

	Galaxies - Information and Observations
		NGC 5557 is a 12.2 magnitude galaxy in Bootes.
		NGC 5529 is barely visible at 70x, on the charts it appears very elongated but seen through the eyepiece it is round and very small.
		NGC 5350, NGC 5354 and NGC 5353 in Canes Venatici form an interesting group, three 12.5 magnitude galaxies clustered in a space of five arcminutes.
	www.nightskyinfo.com /galaxies (643 words)

	Seyfert Galaxy NGC 7742 - Wikipedia, the free encyclopedia
		Seyfert Galaxy NGC 7742 imaged by the Hubble Space Telescope.
		The Seyfert Galaxy NGC 7742 (also known as Galaxy NGC 7742 or NGC 7742) is the designation for a Type 2 Seyfert galaxy and a spiral galaxy that lies approximately 22 mega-parsecs (72 million light-years) away from Earth in the Pegasus constellation.
		This galaxy shows evidence of highly ionized atoms because of the spectrum of its intensely luminous nucleus.
	en.wikipedia.org /wiki/NGC_7742 (124 words)

	Astrocyclopaedia.com-GALAXY PICTURE GALLERY
		The core of NGC 7742 is the large yellow "yolk" in the center of the image.
		NGC 1808 is a prominent radio source, and has been detected at frequencies from 0.03 to 14.8 GHz (Haynes, 1975, Large, 1981, Ekers, 1989).
		NGC 4622 is a rare example of a spiral galaxy with arms pointing in opposite directions.
	www.geocities.com /astrocyclopaedia/galaxy1.htm (3423 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)

	Seyfert Galaxies (Site not responding. Last check: 2007-10-28)
		Seyfert galaxy NGC 4151 has been in the spotlight, because of the massive amount of energy being projected into the surrounding area.
		A face on view of another Seyfert galaxy NGC 7742 gives an interesting visual effect, a "sunny side up egg" is what this small galaxy looks like from its prominent yellow center and white outer rings.
		NGC 7742 is classified as a Seyfert 2 galaxy located in the constellation Pegasus.
	campus.lakeforest.edu /~bell/astro/meghan/SEYFERT2.HTM (675 words)

	Views of PEGASUS
		NGC 7625 Faint, pretty small, not brighter in the middle and has a bright star in the field at 100X.
		NGC 7741 Pretty faint, very elongated, round, somewhat brighter in the middle, there is a double star on the NW side at 135X.
		NGC 7742 Pretty bright, pretty small, round, pretty suddenly brighter in the middle with an almost stellar nucleus at 135X.
	www.saguaroastro.org /content/obsnotes/PEGASUS.htm (1216 words)

	Hubble Heritage Archive - 1998
		October's third Hubble Heritage image is of NGC 7635, AKA the Bubble Nebula, a nebula that is being shaped by a young star in its center.
		November's Hubble Heritage image is of NGC 3132, AKA the Eight-Burst Nebula, AKA the Southern Ring Nebula, a planetary nebula.
		NGC 253 is an almost edge-on spiral galaxy, and it is one of the nearest galaxies beyond our Local Group (a small cluster of about 30 galaxies that contains the Milky Way and Andromeda galaxies).
	burro.astr.cwru.edu /stu/advanced/archive_hst_1998.html (886 words)

	NASA's Observatorium--Image Gallery: Galaxies (Site not responding. Last check: 2007-10-28)
		The horizontal line passing through the image is from the light generated by the powerful fl hole at the center of NGC 4151.
		Spiral galaxy NGC 7742 is not a run-of-the-mill spiral galaxy.
		It is known to be a Seyfert 2 active galaxy, a type of galaxy that is probably powered by a fl hole residing in its core.
	observe.arc.nasa.gov /nasa/gallery/image_gallery/universe/universe_gal4.html (151 words)

	Beyond Our Galaxy
		NGC 4314 is one of the nearest (only 40 million light-years away in the constellation Coma Berenices) examples of a galaxy with a ring of infant stars close to the core.
		This is a Hubble Space Telescope image (left) of a vast nebula called NGC 604, which lies in the neighboring spiral galaxy M33, located 2.7 million light-years away in the constellation Triangulum.
		NGC 4214 contains a multitude of faint stars covering most of the frame, but the picture is dominated by filigreed clouds of glowing gas surrounding bright stellar clusters.
	www.cosmiclight.com /imagegalleries/beyond.htm (4359 words)

	APOD: 2003 July 26 - Spiral Galaxy NGC 7742 (Site not responding. Last check: 2007-10-28)
		In fact, ringed by blue-tinted star forming regions and faintly visible spiral arms, the yolk-yellow center of this face-on spiral galaxy, NGC 7742, is about 3,000 light-years across.
		constellation Pegasus, NGC 7742 is known to be
		tremendous brightness of Seyferts can change over periods of just days to months and galaxies like NGC 7742 are suspected of harboring massive fl holes at their cores.
	antwrp.gsfc.nasa.gov /apod/ap030726.html (151 words)

	Image of the Day
		This spiral, named NGC 7742, is far smaller, with compact and brilliant features that led astronomers to liken it to a frying egg.
		The arms are made visible by the star formation within them, which is less prevalent than in the inner ring but more pronounced than in the dark, emptier regions between the arms.
		NGC 7742 is about 72 million light years away.
	www.space.com /imageoftheday/image_of_day_040212.html (202 words)

	Pets Hub - View Single Post - Space Pictures
		The small spiral galaxy NGC 7742 is probably powered by a fl hole residing in its core.
		The core of NGC 7742 is the large yellow "yolk" in the center of this fried-egg image.
		The nebula is a prime area for starbirth in an arm of the spiral galaxy M33.
	www.petshub.com /forums/showpost.php?p=25202&postcount=2 (326 words)

	Gallery8
		NGC 5194 with a lot of short Branchings
		NGC 4414 with circled Acceleration-Ring and a lot of Winding-Arms
		NGC 4622, Back-Spin-Galaxy with Acceleration-Ring and a Loop
	www.ngc1365.de /gallery8.htm (105 words)

	Peg - Pegasus (Site not responding. Last check: 2007-10-28)
		The quintet of rather distant galaxies--NGC 7317, NGC 7318A, NGC 7318B, NGC 7319, NGC 7320--is an enigma that has been the subject of considerable speculation and controversy.
		It is a faint background object lying adjacent to NGC 7332 in the telescopic field.
		The visual impression of this system is not unlike that of the other notable Pegasus galaxy, NGC 7331.
	mypage.bluewin.ch /horo/ngc/peg.htm (620 words)

	spiral structure: flocculent & grand-design (Site not responding. Last check: 2007-10-28)
		The Seyfert type spiral galaxy NGC 7742 (left) shows an inner ring of star formation with flocculent spiral structure made up of small spiral segments but no real traceable spiral arms.
		The normal spiral galaxy NGC 4062 (right) is also classified a having flocculent spiral structure, but also shows some grand-design structure.
		The other normal spiral galaxy NGC 5248 (right) is also a good example of grand-design spiral structure.
	www.ngcsu.edu /academic/sciences/physics/jones/astr1020home/spiralstructure2.html (98 words)

	[No title]
		The small spiral galaxy NGC 7742 is known as a Seyfert 2 active galaxy, a type of galaxy that is probably powered by a fl hole residing in its core.
		The core of this galaxy is the large yellow "yolk" in the center of the image.
		The lumpy, thick ring around this core is an area of active starbirth.
	www.angelfire.com /rock3/logman7585/NGC_7742.html (59 words)

	Astronomical Observations of Larry Robinson
		NGC 7492 in 13" F4.5 with 25mm is a diffuse globular next to a triangle of stars.
		Then observed NGC 288 big and misty globular cluster mag 8.1 13.8’ later in Ron’s scope he magnified the image and we could see the individual stars.
		NGC 7785 in Pisces was Ron’s next target somewhat edge on in a triangle of stars bright core.
	btboar.tripod.com /obs10597.html (846 words)

	Sea and Sky's Sky Gallery: Spiral Galaxy NGC 7742
		Sea and Sky's Sky Gallery: Spiral Galaxy NGC 7742
		NGC 7742 is a spiral galaxy seen face-on.
		Astronomers believe it may be powered by a massive fl hole located in the galaxy's central core.
	www.seasky.org /skygallery/skygallery_03_25.html (64 words)

	Cosmic Bar Codes
		This figure is the X-ray spectrum of the central region of the galaxy, NGC 5548.
		Like NGC 5548, this galaxy is a Seyfert galaxy - a type of active spiral galaxy with a center or nucleus that is very bright at visible wavelengths.
		Galaxies like NGC 7742 and 5548 are thought to harbor massive fl holes at their cores.
	science.nasa.gov /headlines/y2000/ast22feb_1m.htm (793 words)

	Great quantities of missing mass are hidden in images
		Image source for tightly wound spiral galaxy Ngc 7742.
		In spiral galaxy Ngc 7742, notice how many tightly wound arms there are around the spiral.
		The original cinderella image shows two detached red flyers which are actually the ends of opposedly curved tubes of dim tenuous glowing material.
	www.cosmicastronomy.com /hidden.htm (1497 words)

	[No title] (Site not responding. Last check: 2007-10-28)
		Inspection of earlier LOSS observations of NGC 7742 reveals the presence of this object since Feb. 15, before it disappeared behind the sun.
		Confirmation of SN 1993T was also made by Aviles from a CCD V image obtained on June 5.38.
		SUPERNOVA 1993J IN NGC 3031 Further photoelectric photometry by H. Mikuz, B. Dintinjana, and T. Zwitter, Ljubljana, Slovenia (cf.
	astron.berkeley.edu /~bait/pubs/iauc5812 (326 words)

	62127 (Site not responding. Last check: 2007-10-28)
		Because of their faintness, little is known about the nature of low-luminosity Seyfert galaxies, particularly Seyfert 2 galaxies since the intrinsic continuum can often only be directly observed above 2 keV.
		We propose to observe with ASCA the low-luminosity Seyfert 2 galaxies NGC 2655, NGC 7742, and NGC 4725 as part of a multiwavelength study of low-luminosity AGN.
		NGC 2655 and NGC7743 are two of the brightest Seyfert 2s in our sample in Halpha and NGC 4725 has been detected by ROSAT and in the UV by HST.
	heasarc.gsfc.nasa.gov /docs/asca/ao6/abs/62127.html (119 words)

	TA e-circular (Site not responding. Last check: 2007-10-28)
		Treffers, B. Leibundgut, and A. Filippenko, University of California at Berkeley; and M. Richmond, Princeton University, report the discovery of a probable supernova in NGC 7742 (R.A. 23h41m43s, Decl.
		IAUC 5812 SUPERNOVA 1993J IN NGC 3031 Recently the supernova has been in a plateau phase and there is a possibility that when this ends the decline may be very sharp although given the unique nature of the light curve to date it is by no means certain what will happen next.
		To date over 700 visual observation have been accepted into the database and we are currently reviewing a further 200 estimates secured from either CCD or conventional photography.
	www.theastronomer.org /tacirc/1993/E0748.txt (469 words)

	JCA Outreach: X-ray Observations of AGN
		In some cases, the size of the AGN is smaller than the size of our solar system.
		HST image (in the optical band) of the AGN NGC 7742.
		Although the flhole itself is invisible (by definition), gas accreting, or falling, onto a flhole becomes hot (possibly similar to how a meteor gets hot falling through the Earth's atmosphere) and some of this energy escapes for us to see.
	www.jca.umbc.edu /~george/html/science/outreach/agn_xrays.shtml (333 words)

	Galaxies
		NGC 300 closeup - "stars as numerous as grains of sand"
		Nucleus of NGC 4261 (1.2 Billion solar masses)
		Seyfert Galaxy NGC 5728 (note jets from nucleus)
	www.gpc.edu /~bskelton/1020/galaxies/galaxies.html (167 words)

	APOD: October 23, 1998 - Seyfert Galaxy NGC 7742 (Site not responding. Last check: 2007-10-28)
		APOD: October 23, 1998 - Seyfert Galaxy NGC 7742
		About 72 million light-years away in the constellation Pegasus, NGC 7742 is known to be
		tremendous brightness of Seyferts can change over periods of just days to months and galaxies like NGC 7742 are suspected of harboring
	antwrp.gsfc.nasa.gov /apod/ap981023.html (134 words)

	Observations made in the constellation Pegasus
		With a magnitude of 15.1 to 15.5 SN 2002dp was by far the dimmest exploding star that I have ever viewed.
		NGC 7448 is far larger and brighter than a group of 12th and 13th magnitude galaxies, including NGC 7463, NGC 7464, and NGC 7465, that lie to the east.
		It was seen as an elongated streak through the ASH 17" f/15 classical Cassegrain (202x) and earlier in the night through the ASH 12.5" f/6.5 Cave Newtonian.
	www.lies.com /aaol/view_obs.cgi?con=Peg (2545 words)

	Novinky z HST
		Obøí hvìzdná továrna v blízké galaxii NGC 6822
		Galaxie NGC 1365 v kupe galaxii v souhvezdi Fornax
		Prachovy disk kolem cerne diry v galaxii NGC 4162
	astro.sci.muni.cz /hstnew.html (668 words)

	UNIVERSAL ENLIGHTENMENT
		The image to the right is Hubble's face-on snapshot of the small spiral galaxy NGC 7742.
		The Hubble telescope has spied a giant celestial "eye," known as planetary nebula NGC 6751.
		Glowing in the constellation Aquila, the nebula is a cloud of gas ejected several thousand years ago from the hot star visible in its center.
	casa.colorado.edu /TourofCASA/InTheMedia/dcamera_57_2000.shtml (1389 words)

	NGC 4 Star Images, Outer Sky Photos Deep Space Pictures
		NGC 2244, Open Cluster in Rosetta Nebula, Russell Croman
		NGC 4945, Dusty Southern Spiral Galaxy, AAT 101
		NGC 7048 Planetary, Bruce Balick, AIT ¶¶, Cygnus
	www.biochem.szote.u-szeged.hu /astrojan/ngc4t.htm (162 words)

	APOD: 2003 July 26 - Spiral Galaxy NGC 7742 (Site not responding. Last check: 2007-10-28)
		Explanation: This might resemble a fried egg you've had for breakfast, but it's actually much larger.
		In fact, ringed by blue-tinted star forming regions and faintly visible spiral arms, the yolk-yellow centre of this face-on spiral galaxy, NGC 7742, is about 3,000 light-years across.
		tremendous brightness of Seyferts can change over periods of just days to months and galaxies like NGC 7742 are suspected of harboring massive fl holes at their cores.
	www.star.ucl.ac.uk /~apod/apod/ap030726.html (151 words)

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