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Topic: NGC 5904

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	Astron. Astrophys. 362, 953-958 (2000)
		NGC 6712 has a wide HB colour range, similar to those of the blue tail clusters NGC 6388 and NGC 6441 (Rich et al.
		= 0.0, implying that the reddening of NGC 6712 is the same as that of NGC 6171 (H96), estimated to be E(B-V) = 0.33.
		NGC 6712 is thus one of the few globular clusters presenting Long Period Variables, which is an indication that it is rather metal rich (Rosino 1978).
	aa.springer.de /papers/0362003/2300953/sc4.htm (956 words)

	Cielo Sur - Objetos Messier
		M9: NGC 6333.Cúmulo globular, se encuentra en la constelación de Ofiuco, tiene una magnitud de 8.0, se encuentra a unos 25.000 años luz.
		Se encuentra en la constelación de Canis Venatici (Los Lebreles), está unida a una galaxia compañera (NGC 5125) por un puente de materia brillante.
		Cúmulo globular (NGC 6266), magnitud 7.0, en la constelación de Ofiuco, se encuentra a 26.000 años luz.
	www.cielosur.com /messier.php (7286 words)

	Deepsky observing report M16, M17, M18, M24, M22, M8, M11, IC 4756, NGC 6633, NGC 253, NGC 247, NGC 188, NGC 891
		NGC 253 can be found about 7 to 8° to the south of this 2nd magnitude star.
		NGC 253 is 30′x 7′, with a visual magnitude of 7.6 and a surface brightness of 13.2.
		NGC 891 lies inside this trapezoid, just to the northwest of the most eastern star (on the image below, South is up and West is to the Left).
	www.backyard-astro.com /deepsky/2003_09_26/ITT.html (2672 words)

	Views of SERPENS
		NGC 5953 and 5954 This is a contact galaxy pair and the two galaxies could just barely be split into separate objects at 220X.
		NGC 5956 Faint, small, round, bright middle, flanked by two 13th mag stars on either side to the east and west at 135X.
		NGC 6118 Pretty faint, pretty large, somewhat brighter in the middle and elongated 2.5 X 1 in PA 60 at 100X.
	www.saguaroastro.org /content/obsnotes/SERPENS.htm (1556 words)

	110 Messier Objects Photos. M Object Images Galaxy Pictures
		M17, NGC 6618, Lobster Nebulosity, APD 96 08 29
		M27, NGC 6853, Dumbbell Nebel, APD 98 10 09
		NGC 4486, M87, Jet from Virgo A, APD 00 07 06
	www.biochem.szote.u-szeged.hu /astrojan/messiert.htm (349 words)

	Messier Object 5
		Globular cluster Messier 5 (M5, NGC 5904) was first seen by Gottfried Kirch and his wife Maria Margarethe on May 5, 1702, when they observed a comet, and described as a "nebulous star".
		One of the other variables is a dwarf nova, according to Cecilia Payne-Gaposhkin (she also mentions two more dwarf novae in the globulars M30 and NGC 6712).
		To the west of M5 and up to 110 Virginis is a collection of faint distant galaxies including NGCs 5806, 5811, 5813, 5814, 5831, 5838, 5839, 5845, 5846, 5846A, 5848, 5850, 5854, 5864, 5865, 5869 and 5887, of brightnesses between mag 10.0 and 13.9, mostly requiring larger telescopes.
	www.seds.org /messier/m/m005.html (770 words)

	Globular cluster M 5 (NGC 5904)
		The bright globular cluster Messier 5 (NGC 5904) in Serpens, shown from a 15-second yellow-light (V-band) exposure (in twilight) with a Tektronix 2048x2048 CCD at the prime focus of the 4-meter Mayall telescope of Kitt Peak National Observatory.
		North is at the top and east to the left, for direct comparison with a chart or eyepiece view.
		This is one of the brighter globular clusters visible from the northern hemisphere, with a listed magnitude of 5.8 (not to be more specific, that's from the Sky Publishing Messier Card).
	www.racine.ra.it /planet/testi/Foto/m5.htm (120 words)

	Gary's Amateur Astronomy
		NGC 5272; Canes Venatici; 13h 42.2m; +28 23'
		A member of the Virgo Galaxy Cluster along with NGC 4467, NGC 4470 and a faint dwarf galaxy.
		NGC 5024; Coma Berenices; 13h 12.9m; +18 10'
	home.comcast.net /~astrohammer/Observingmessier.htm (916 words)

	CCD images
		M17 NGC 6618 the Omega Nebula in Sagittarius
		M20 NGC 6514 the Trifid Nebula in Sagittarius
		M8 NGC 6523 the Lagoon Nebula in Sagittarius
	www.mv.com /ipusers/astron/ccd_images.htm (411 words)

	Astronomy Online - Messier Cross Reference
		It is the "modern" Messier Catalog for amateur astronomers that seek deep sky delights that are both challenging and rewarding; however there are no Messier listings in the Caldwell Catalog.
		An additional listing is the column "Finest NGC Object" list, a list compiled by Alan Dyer (a 'competitive' list to the Caldwell Catalog).
		While there are no Caldwell or Finest NGC counterparts to the Messier Objects, the table is filled in for completeness (and so you do not have to search the web to see if there are counterpart entries):
	astronomyonline.org /Astrophotography/MessierTable.asp (319 words)

	Globular Clusters (gc) - IceInSpace Forums
		NGC 6397 is the nearest GC, only 2.2 kpc away = 7.2 klyrs
		Half of the globular clusters have NGC numbers between 6000 and 7000.
		NGC 7099 M 30 has the highest concentration.
	www.iceinspace.com.au /forum/showthread.php?t=14088 (271 words)

	DSS Images for NGC 5900 thru NGC 5999
		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_n5900.asp (300 words)

	Comparison with Cluster Data (Site not responding. Last check: 2007-10-15)
		The clusters examined here are M 5 (=NGC 5904), 47 Tuc (=NGC 104), NGC 6528, and M 67 (=NGC 2682).
		Abundances for NGC 6528 are averages of the determinations by Carretta et al.
		Another important difference is the one between the abundance pattern of NGC 6528 and that of library stars of near-solar metallicity.
	astsun.astro.virginia.edu /~rps7v/Models/ms/node25.html (874 words)

	2 The cluster sample and age-dating method (Site not responding. Last check: 2007-10-15)
		The reference clusters are, respectively, M 15 (NGC 7078), M 3 (NGC 5272), NGC 6171 and 47 Tuc (NGC 104).
		Due to the small [Fe/H] differences with respect to SW98, the cluster NGC 6171 has now moved to the third metallicity group where it has replaced M 5 (NGC 5904) as the reference cluster.
		It is interesting to determine the age difference for two classic second-parameter pairs, namely NGC 288-NGC 362 and M 3-M 13 (NGC 6205), both contained in our sample.
	aanda.u-strasbg.fr:2002 /papers/aa/full/2002/23/aah3508/node2.html (2129 words)

	(IAAC) Obj: M 5 (NGC 5904) - Inst: 8" f/6 Newton, alt-az mount (Site not responding. Last check: 2007-10-15)
		(IAAC) Obj: M 5 = NGC 5904 - Inst: 8" f/6 Newton, alt-az mount
		Subject: (IAAC) Obj: M 5 = NGC 5904 - Inst: 8" f/6 Newton, alt-az mount
		Prev: (IAAC) Obj: NGC 1 - Inst: 17.5" f/4.4 dob, 13" f/4.5 dob
	www.visualdeepsky.org /netastrocatalog/msg00847.html (193 words)

	Serpens
		Another faint globular, larger and brighter than NGC 6535.
		NGC 6027 is 0.4 x 0.2 arc minutes in size.
		The whole grouping fits in an area only 2.2 x 1.2 arc minutes.
	calgary.rasc.ca /constellations/serpens.htm (253 words)

	M5
		MESSIER INDEX - NGC INDEX - NAME INDEX
		Messier object: M5 (New General Catalog) number: NGC 5904
		Use Test patterns to calibrate monitor brightness, contrast, height and width
	www.stargazing.net /david/messier/m5.html (136 words)

	RedOrbit - Gallery - M 5 (Site not responding. Last check: 2007-10-15)
		Globular cluster M5 was first seen by Gottfried Kirch and his wife Maria Margarethe on May 5, 1702, when they observed a comet, and described as a "nebulous star".
		One of the other variables is a dwarf nova, according to Cecilia Payne-Gaposhkin (she also mentions two more dwarf novae in the globulars M30 and NGC 6712).
		To the west of M5 and up to 110 Virginis is a collection of faint distant galaxies including NGCs 5806, 5811, 5813, 5814, 5831, 5838, 5839, 5845, 5846, 5846A, 5848, 5850, 5854, 5864, 5865, 5869 and 5887, of brightnesses between mag 10.0 and 13.9, mostly requiring larger telescopes.
	www.redorbit.com /images/gallery/messier_objects/m_5/104/106/index.html (784 words)

	WAS List of 130 Deep Sky Objects (Site not responding. Last check: 2007-10-15)
		NGC 7635, NGC 457, NGC 7789, NGC 7654
		NGC 6633, NGC 6218 (M 12), NGC 6254 (M 10), NGC 6266 (M 62), NGC 6273 (M 19), NGC 6402 (M 14), NGC 6333 (M 9), NGC 6171 (M 107), NGC 6293, NGC 6572
		NGC 4594 (M 104), NGC 4472 (M 49), NGC 4486 (M 87), NGC 4649 (M 60), NGC 4406 (M 86), NGC 4374 (M 84), NGC 4569 (M 90), NGC 4526, NGC 4579 (M 58), NGC 4621 (M 59)
	www.westminsterastro.org /projects/was130.htm (6193 words)

	Nomenclature of Celestial Objects (Result I)
		Table 1: NGC 5904 SB 1-NNN> (Nos 1-1 to 1-105).
		Table 4: NGC 5904 SB 4-NNN> (Nos 4-1 to 4-446).
		Table 3: The RRLyrae stars are 'Cl* NGC 5904 SAW VNNN' in SIMBAD.
	cdsweb.u-strasbg.fr /cgi-bin/Dic-Simbad?SB (216 words)

	[45.05] FUSE Observations of the UV-Bright Star ZNG 1 in M5 (NGC 5904) (Site not responding. Last check: 2007-10-15)
		To investigate this phenomenon, we have observed several UV-bright stars in globular clusters with FUSE, the Far Ultraviolet Spectroscopic Explorer.
		In this poster, we present first results for the post-AGB star ZNG 1 in M5 (NGC 5904).
		Previous studies have shown the star to have an effective temperature of about 41,000 K and a surface gravity of log g = 4.5.
	www.aas.org /publications/baas/v33n2/aas198/388.htm (203 words)

	Spring 2000--Cousin Ricky's Astronomy Logs
		As best as I can determine, the nebulosity (NGC 6523) is too dim for the naked eye.
		I had NGC 4976 and NGC 4945 written down and then crossed out for this Date.
		During the search, I ran across what looked like open clusters, but I could only find galaxies NGC 4976 and NGC 4945 in the references I had.
	cac.uvi.edu /staff/rc3/astro/logs/log00b.html (623 words)

	The Astronomical Zoo
		M20 (NGC 6514) "The Trifid Nebula" (pretty dim - you might need to play with your monitor)
		Tarantula Nebula (NGC 2070) - a star-forming region in the Magellanic Clouds
		M87 (NGC 4486) - center of the Virgo cluster of galaxies
	mintaka.sdsu.edu /faculty/erics/web/azoo.html (154 words)

	NGC 5094 (Messier 5) (Site not responding. Last check: 2007-10-15)
		These stars affect the overall colour of the cluster significantly, making its integrated light slightly bluer than that of the Sun.
		Entry from NGC 2000.0 (R.W. Sinnott, Ed.) © Sky Publishing Corporation, 1988:
		NGC 5904 Gb 15 18.6 +02 05 s Ser 17.45.8 !!, glob.
	www.aao.gov.au /images/captions/aat070.html (162 words)

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