NGC1042

NGC 1128

NGC3031

NGC3054

SABbc

NGC 1 seen by the SDSS

NGC 105 is a spiral galaxy estimated to be about 240 million light-years away in the constellation of Pisces. It was discovered by Édouard Stephan in 1884 and its apparent magnitude is 14.1.

NGC 131

NGC 1-999

PGC 1844, UGC 301.

NGC1808

NGC7000

NGC1068

NGC185

NGC 10

Fornax A, PGC 12651, Arp 154

NGC 123 is a non-existent object historically located in the constellation Cetus.

PGC 012626

NGC 1058

SBab

NGC 1023 group

NGC 134

NGC2261

NGC 122 is a non-existent object historically located in the constellation Cetus.

NGC247

NGC122

"Faint, irregular figure, a little brighter middle."

NGC 1027

NGC2500

NGC1409

S a? pec

NGC 1288 is an intermediate barred spiral galaxy located about 196 million light years away in the constellation Fornax. In the nineteenth century, English astronomer John Herschel described it as "very faint, large, round, very gradually little brighter middle." The morphological classification of SABc(rs) indicates weak bar structure across the nucleus (SAB), an incomplete inner ring orbiting outside the bar (rs), and the multiple spiral arms are moderately wound (c). The spiral arms branch at intervals of 120° at a radius of 30″ from the nucleus. The galaxy is most likely surrounded by a dark matter halo, giving it a mass-to-light ratio of 14 M☉/L☉.On July 17, 2006, a supernova with a magnitude of 16.1 was imaged in this galaxy from Pretoria, South Africa, at 12″ east and 2″ of the galactic core. Designated SN 2006dr, it was determined to be a type Ia supernova.

NGC108

NGC1532

NGC132

NGC3

NGBR

NGC2023

NGC 1269

NGC 108 is a lenticular galaxy that is located at approximately 220 million light-years away in the constellation of Andromeda. It was discovered by William Herschel on September 11, 1784.

NGC6101

NGC188

NGC2536

Image from 2MASS

NGC 1087

ESO

SABc

NGC 119

NGACs, or New South Wales Greenhouse gas Abatement Certificates, are kind of Carbon credit issued by the New South Wales State Government of Australia.

NGC 130

SA0+P

NGC 1260 imaged by the Hubble Space Telescope

NGC3180

NGC 1

NGC123

NGC5139

Abell

NGC 118

SB0/a

NGC 11

NGC 1003 is a spiral galaxy located in the Perseus constellation about 28 million light years from the Milky Way. It was discovered by the German-British astronomer William Herschel in 1784.

NGC 1245

NGC 132

NGAL

NGC3077

NGC1818

NGC 13

NGC7027

NGC 1058 is a Seyfert Type 2 galaxy in the NGC 1023 Group, appearing in the Perseus constellation. It is approximately 27.4 million light years from Earth and has an apparent magnitude of 11.82. It is receding from Earth at 518 kilometers per second (322 mi/s), and at 629 kilometers per second (391 mi/s) relative to the Milky Way.

NGC 135

NGC 125 (also known as PGC 1772) is a lenticular galaxy located in the constellation Pisces. It is designated as subclass Sa Ring in the galaxy morphological classification scheme. It lies approximately 235 million light-years away.

NGC 1003 as seen through the Hubble Space telescope.

NGC 1169

NGC2447

NGC2287

NGC1904

NGC2736

NGC 1342

NGC1502

NGC3184

NGC 103
open cluster

NGC1531

NGC 117

NGC1234

NGC1316

NGC288

NGC 1134

NGC2683

NGC2363

NGC2080

NGC 1169 (UGC 2503) is an intermediate barred spiral galaxy in the constellation of Perseus. NGC 1169 has a reddish center, indicating the region is dominated by older stars. In contrast, the outer ring contains larger blue-white stars, a sign of recent star formation. The entire galaxy is rotating at approximately 265 km/s NGC 1169 was discovered on December 11, 1786 by William Herschel. Measurements of its distance range from 20.9 Mpc - 49.7 Mpc with an average of 35.1 Mpc.

NGC120

NGC17

NGC 100

NGC 1058 imaged by the Hubble Space Telescope

UGC 00292, PGC 1791,

NGC 1260 is a spiral or lenticular galaxy in the constellation Perseus. In 2006, it was home to the second brightest supernova in the observable universe, supernova SN 2006gy.

This composite image of NGC 1291 is processed primarily from data collected by NASA's Galaxy Evolution Explorer in December 2003. The blue in this image is ultraviolet light captured by GALEX's long wavelength detector, the green is ultraviolet light detected by its short wavelength detector, and the red in the image is visible light courtesy of data from the Cerro Tololo Inter-American Observatory in Chile.

NGC117

NGC292

NGBA

PGC1813 and 199360

NGC103

NGC206

NGC 1300

NGC2371

NGC3267

E/SA0?

NGC 103 is a small group of stars partially visible in an 8" amateur telescope under moderately light polluted skies. It is roughly 4600 light years from the Sun.

NGC 1398

NGC 110 is an open star cluster located in constellation Cassiopeia, discovered by English astronomer John Fredrick William Herschel on October 29, 1831.It is unknown if the members are physically related, or if the cluster exists at all. It is barely visible against the background sky, and the primary stars seem to be at various distances. If the cluster does exist, it is at least 2,000 light years away.

NGC1039

NGC 1316

NGC7293

NGB (disambiguation)

NGC1073

NGC2541

NGC2362

NGC 12

NGC4594

NGC 1260

NGBC

NGCC

NGC2477

NGC 131, is a spiral galaxy, was discovered on September 25, 1834 by John Herschel. This galaxy belongs in the NGC 134 group of galaxies: NGC 115, NGC 148, NGC 150, PGC 2000 (often confused with IC 1554), IC 1555, and PGC 2044.

NGC 1234

NGC1982

NGB

NGC 134 imaged using the ESO's Very Large Telescope at Paranal in 2007.

SBb

NGATS

S0 pec

Hodge 3

NGC1975

NGC250

NGC7686

UGC 309, PGC 1888

NGC1788

A Hubble Space Telescope image of NGC 1309.
NGC 1309

NGCA (disambiguation)

S0/a

NGC 120

NGC278

SAbc

NGC7331

NGC2976

NGC3260

NGC2516

NGC2867

NGC2244

NGC 1003

NGC-246

NGC1

NGC3351

NGC2422

PGC 1772, UGC 286

NGC 1265

NGC1275

Sbc

NGC1912

NGC 1169 (UGC 2503) is an intermediate barred spiral galaxy in the constellation of Perseus. NGC 1169 has a reddish center, indicating the region is dominated by older stars. In contrast, the outer ring contains larger blue-white stars, a sign of recent star formation. The entire galaxy is rotating at approximately 265 km/s NGC 1169 was discovered on December 11, 1786 by William Herschel. Measurements of its distance range from 20.9 Mpc - 49.7 Mpc with an average of 35.1 Mpc. and exhibits a slight ring structure.

NGC281

NGC1427

NGC 1234 is a peculiar barred spiral galaxy exhibiting a ring structure in the constellation Eridanus, discovered by Francis Preserved Leavenworth in 1886.

NGC 113 is a lenticular galaxy located in the constellation Cetus.It was discovered by German astronomer, Ernst Wilhelm Leberecht Tempel, on August 27, 1876. The galaxy lies approximately 210 Million light-years from earth, and is about 80,000 light-years in diameter.

NGC246

PGC 12219

NGC221

NGC1309

NGC 118 is a spiral galaxy of type S (rs)a? pec with an apparent magnitude of 13.6 located in the constellation Cetus.

NGC3195

NGC7319

SBcd pec

NGC2237

PGC 012209,

NGC6543

NGC104

NGC 123

Perseus

NGAT

ESO 482-22

NGC 117 is a lenticular galaxy of type S0(r)a with a magnitude of 14.3 in the constellation Cetus.

NGC 1234 imaged by GALEX

NGC 109 is a spiral galaxy estimated to be about 240 million light-years away in the constellation of Andromeda. It was discovered by Heinrich d'Arrest in 1861 and its magnitude is 13.7.

E/SAo

NGC 1032

NGC 1087 is an intermediate spiral galaxy in Cetus. The central bar/core is very small with many irregular features in the surrounding disk of material. With the many strange features of NGC 1087, its true nature is still uncertain. It has an extremely small nucleus and a very short stellar bar. Unlike most barred galaxies, the bar apparently has some new star-formation taking place. There is a multiple spiral structure defined more by the dust lanes than by luminous matter.

NGC3079

NGC 110

NGC3115

NGC253

NGC3982

Credit: HST/NASA/ESA.

NGC2372

NGC 113

NGC2323

NGC1999

NGC1410

NGC130

Huge bar-shaped core and two spiral arms

NGC2360

Very bright at radio 1.4 GHz

NGC 111 is the designated name for a lost or non-existent object in the constellation Cetus.

NGC 130, a lenticular galaxy, was discovered on November 4, 1850 by Bindon Stoney, the very same day he discovered NGC 126 and 127. This galaxy belongs in the NGC 128 group of galaxies.

NGC 100 is a galaxy in the constellation Pisces. It has an apparent magnitude of 13.2. It is located at RA 24min 2.6s, Dec +16°29'11". It was first discovered on 10 November 1885 by American astronomer Lewis Swift.

NGC 111

NGC 1027 is an open cluster in the constellation Cassiopeia. It was discovered by William Herschel in 1787. It is visible at the eastern part of the constellation, between two emission nebulae, the Heart and Soul Nebula. However, it is not physically associated with the two nebulae, lying in the foreground, about 3,000 light years away from the Solar System.

HST/NASA/ESA.

NGC 1023 Group

NGC 137

NGC/IC Project

NGC1427A

After Galaxies Collide

NGC 120 is a lenticuluar galaxy of type SB0? pec? with an apparent magnitude of 13.4 located in the constellation Cetus.

NGC7023

NGC111

The NGC 1023 group is a group of galaxies about 20.6 million light-years away from Earth. The group resides in the Canes Venatici Cloud in the Virgo Supercluster.

NGC290

NGC 1156

NGC6820 and NGC6823

NGC5866

NGC3268

NGC1435

NGC 116 is a possibly lost or non-existent object in the constellation Cetus. This object is up for debate and has been considered to possibly be PGC 1671.

NGC2787

NGC 1156 is a dwarf irregular galaxy in the Aries constellation of the type ibm. It is considered a Magellanic-type irregular. The galaxy has a larger than average core, and contains zones of contra-rotating gas. The counter-rotation is thought to be the result of tidal interactions with another gas rich galaxy some time in the past.The AGES survey has discovered a candidate dark galaxy close to NGC 1156, one of only a few so far found.It has a H II nucleus.

NGC 1049 by Hubble space telescope

Loose galaxy group

NGC1559

NGC 1134 is a spiral galaxy in the Aries constellation. It has a highly inclined disk, with respect to the line of sight from Earth. There is a weak outer extension of the spiral structure in this galaxy. It has been listed in the Arp Atlas of Peculiar Galaxies (Arp number 200), under the "Galaxies with material ejected from nuclei" section. NGC 1134 is classified as a galaxy with reduced surface brightness, and it possesses a distinct bulge in its centre, as judged by photometric analysis.

NGC 108

NGC3226

NGC3344

NGC 13 2MASS

NGC2437

NGC 101 is a spiral galaxy estimated to be about 150 million light-years away in the constellation of Sculptor. It was discovered by John Herschel in 1834 and its magnitude is 12.8.

NGC 12 is a spiral galaxy in the Pisces constellation.

NGC3227

NGB Airport

PGC 1671

NGC2174

NGC 1265 is a Fanaroff and Riley class 1 radio galaxy located in the constellation Perseus, a member of the Perseus Cluster.

NGC116

NGC 125

NGC 128

NGC

NGC 122

NGC 1398 is an isolated barred spiral galaxy exhibiting a double ring structure. It is located 65 million light years from the Earth, in the constellation of Fornax. The galaxy, with a diameter of 135,000 light years, is slightly larger than the Milky Way. Over 100 billion stars are in the galaxy. It was first discovered by Friedrich Winnecke of Karlsruhe, Germany, on 17 December 1868, while he was searching for comets.

NGC2099

NGC1960

NGC 128 is a lenticular galaxy in the constellation Pisces. It is approximately 190 million light-years from earth and has a diameter of about 165,000 light years.

NGC 107

PGC 1813 and 199360

NGC 137 is a lenticular galaxy in the constellation of Pisces. It was discovered by William Herschel on November 23, 1785.

NGC 1309 is a spiral galaxy located approximately 120 million light-years away, appearing in the constellation Eridanus. It is about 75,000 light-years across, and is about 3/4s the width of the Milky Way. Its shape is classified as SA(s)bc, meaning that it has moderately wound spiral arms and no ring. Bright blue areas of star formation can be seen in the spiral arms, while the yellowish central nucleus contains older-population stars.

NGC 1027 is an open cluster in the constellation Cassiopeia. It was discovered by William Herschel in 1787. It is visible at the eastern part of the constellation, between two emission nebulae, the Heart and Soul Nebula. However, it is not physically associated with the two nebulae, lying in the foreground, about 3,000 light years away from the Solar System. The apparent magnitude of the cluster is 6.7 and can be seen with 10x50 binoculars around a 7th magnitude star, which is not however member of the cluster. The brightest member of the cluster has apparent magnitude 9,3.

NGC 1087 is an intermediate spiral galaxy in Cetus. The central bar/core is very small with many irregular features in the surrounding disk of material. With the many strange features of NGC 1087, its true nature is still uncertain. It has an extremely small nucleus and a very short stellar bar. Unlike most barred galaxies, the bar apparently has some new star-formation taking place. There is a multiple spiral structure defined more by the dust lanes than by luminous matter. Overall, the disc has a very low surface brightness. Even though it appears close to another galaxy (NGC 1090), these two galaxies are not interacting and should be considered isolated from one another.NCG 1087 lies near the small M77 (NGC 1068) galaxy group that also includes NGC 936, NGC 1055, and NGC 1090. However, because of its distance, it probably is not an actual group member.Based on the published red shift, (Hubble Constant of 62 km/s per Mpc) a rough distance estimate for NGC 1087 is 80 million light-years, with a diameter of about 86,800 light-years. The Type II Supernova 1995V is the only recorded supernova in NGC 1087.

NGC2366

NGC2022

UGC 2455, PGC 11329

NGC2812

NGC2392

NGC6820

NGC1087

NGC 1169, UGC 2503, PGC 11521

Lenticular galaxy NGC 108

NGC 1245 is an open cluster in the constellation Perseus. It was discovered by William Herschel in 11 December, 1786. It is located 3° southwest of alpha Persei and can be spotted with 10x50 binoculars. The cluster is nearly 1 billion years old. NGC 1245 has about 200 members the brightest of which are of 12th magnitude. The cluster shows evidence of mass segredation and it is possible that it has lost its lower mass members.

NGC2068

NGA GNS

NGC 12 2MASS

NGC 11 is a spiral galaxy located in the Andromeda constellation. It is located at right ascension 00h 08m 42.5s; declination +37° 26′ 53″; under J2000.0 coordinates.

NGC 116

NGC113

IBm

ESO 350-23

NGC1232

NGC7822

NGC 1360

NGC4676

CGCG

inner bar and outer ring structure

NGC1128

NGC2204

NGC 1032 is a spiral galaxy that is about 117 million light-years away in the constellation Cetus.

Image of NGC 1169 taken by Adam Block

NGC1300

NGC2440

NGC1499

NGC118

Binary black hole system 3C 75 contained in the dumbbell shaped galaxy NGC 1128

A Hubble Space Telescope image of NGC 1300.

NGC1365

A Hubble Space Telescope image of NGC 1316.

NGC 1232A

NGC 1134 is a spiral galaxy in the Aries constellation. It has a highly inclined disk, with respect to the line of sight from Earth. There is a weak outer extension of the spiral structure in this galaxy. It has been listed in the Arp Atlas of Peculiar Galaxies (Arp number 200), under the "Galaxies with material ejected from nuclei" section. NGC 1134 is classified as a galaxy with reduced surface brightness, and it possesses a distinct bulge in its centre, as judged by photometric analysis. It has a small and distant companion about 7' to the south.

Barred Spiral Galaxy NGC 1300

NGC 1039

NGC2715

NGC225

NGC 1049

NGC 109

NGC 1049 is a globular cluster located in the Local Group galaxy of Fornax Dwarf, visible in the constellation of Fornax. At a distance of 630,000 light years, it is visible in moderate sized telescopes, while the parent galaxy is nearly invisible. This globular cluster was discovered by John Herschel in the period 1834–1838, while the parent galaxy was discovered in 1938 by Harlow Shapley.

NGA, Washington

OCL291

NGC1850

HST image of NGC 1265

NGC 119 is a lenticuluar galaxy of type E/SA0? pec with an apparent magnitude of 13.0 located in the constellation Phoenix.

NGC 13 is a spiral galaxy in the Andromeda constellation.

NGC 1309 is a spiral galaxy located approximately 120 million light-years away, appearing in the constellation Eridanus. It is about 75,000 light-years across, and is about 3/4s the width of the Milky Way. Its shape is classified as SA(s)bc, meaning that it has moderately wound spiral arms and no ring. Bright blue areas of star formation can be seen in the spiral arms, while the yellowish central nucleus contains older-population stars. NGC 1309 is one of over 200 members of the Eridanus Group of galaxies.

SAB00

NGC 101

NGC (disambiguation)

NGC119

Dumbbell-shaped galaxy

NGC2

NGC2442

NGC 1245 is an open cluster in the constellation Perseus. It was discovered by William Herschel in 11 December, 1786. It is located 3° southwest of alpha Persei and can be spotted with 10x50 binoculars. The cluster is nearly 1 billion years old. NGC 1245 has about 200 members the brightest of which are of 12th magnitude. The cluster shows evidence of mass segredation and it is possible that it has lost its lower mass members. Lying at a distance of 3kpc, the cluster is estimated to be 27 light years across.

NGC 132 is a spiral galaxy in the constellation Cetus. It was discovered by William Herschel.

NGC3201

NGC 107 is a spiral galaxy estimated to be about 280 million light-years away in the constellation of Cetus. It was discovered by Otto Struve in 1866 and its magnitude is 14.2.

PGC 12412

NGC 106 is a lenticular galaxy estimated to be about 270 million light-years away in the constellation of Pisces. It was discovered by Francis Leavenworth in 1886 and its apparent magnitude is 14.5.

NGAC

SBbc

NGC 1128 is a "dumbbell galaxy" in the Abell 400 galaxy cluster. It is the center of the 3C75 radio source and contains two orbiting supermassive black holes that may be merging. Computer simulations indicate that these two black holes will gradually spiral in toward each other until they merge. Lewis Swift is credited with the discovery of NGC 1128 in 1886.

NGC-1128

NGC 1316 (also known as Fornax A) is a lenticular galaxy about 60 million light-years away in the constellation Fornax. NGC 1316 is a radio galaxy. It is the fourth-brightest radio source in the sky (as seen at 1400 MHz).

NGC404

NGC3242

NGC131

NGC 11 2MASS

NGC3223

NGC6823

NGC 1288 is an intermediate barred spiral galaxy located about 196 million light years away in the constellation Fornax. In the nineteenth century, English astronomer John Herschel described it as "very faint, large, round, very gradually little brighter middle." The morphological classification of SABc(rs) indicates weak bar structure across the nucleus (SAB), an incomplete inner ring orbiting outside the bar (rs), and the multiple spiral arms are moderately wound (c).

NGC2169

NGC1705

NGC2632

NGC266 LBV 1

NGC 1300 is a barred spiral galaxy about 61 million light-years away in the constellation Eridanus. The galaxy is about 110,000 light-years across (about 2/3 the size of the Milky Way). It is a member of the Eridanus Cluster, a cluster of 200 galaxies. It was discovered by John Herschel in 1835.In the core of the larger spiral structure of NGC 1300, the nucleus shows a "grand-design" spiral structure that is about 3,300 light-years long. Only galaxies with large-scale bars appear to have these grand-design inner disks — a spiral within a spiral. Models suggest that the gas in a bar can be funneled inwards, and then spiral into the center through the grand-design disk, where it can potentially fuel a central black hole. NGC 1300 is not known to have an active nucleus, indicating that its central black hole is not accreting matter.

NGC2997

NGC2175

NGAD

NGC2346

NGBROI

NGAA

NGC3310

NGCA

NGC2548

NGC660

NGCP

NGC1090

NGCSU Saints

NGC6823 and NGC6820

NGC1973

NGC3132

NGC2682

NGC 1300 galaxy

NGC3281

NGC 1291

SB0? pec?

NGC1427a

NGC2841

SABb

NASA / ESA / S. Larsen

Cetus RA 00 27 11.1, Dec +01 20 02)

NGC2158

NGC2419

NGC 1342 is an open cluster in the constellation Perseus. It was discovered by William Herschel on 28 December 1799. It is located in the south of the constellation, almost halfway between Algol (β Persei) and ζ Persei, away from the plane of the Milky Way. NGC 1342 has an apparent size of 17' and an apparent magnitude of 6.7, marginally visible by naked eye. In 1994, Peña, J. H. and Peniche, R. estimated by the use of photometric data, that the age of the cluster is 400 millions years.

NGC205

Composite image of NGC 1288 taken with the Very Large Telescope. Supernova SN 2006dr is visible just to the left of the nucleus.

PGC1794

NGC3271

NGC 103

NGC2207

IV1p

NGC 1288

NGC1512

NGC2915

NGC300

NGC 1300 is a barred spiral galaxy about 61 million light-years away in the constellation Eridanus. The galaxy is about 110,000 light-years across (about 2/3 the size of the Milky Way). It is a member of the Eridanus Cluster, a cluster of 200 galaxies. It was discovered by John Herschel in 1835.In the core of the larger spiral structure of NGC 1300, the nucleus shows a "grand-design" spiral structure that is about 3,300 light-years long.

NGC 1156 imaged by the Hubble Space Telescope

UGC 2245, PGC 10496

NGC7662

NGA (British trades union)

NGC1097

NGC3372

NGC 106

NGAUS

PGC 1794

NGC1977

NGA Hooters Tour

E/SA0? pec

NGCSU

NGC 10 ESO Schmidt-Telescope

NGC2537

PGC 11188

NGC1265

NGC 105

NGC5128

NGC2547

NGC1055