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Topic: NGC 185

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In the News (Fri 26 Apr 19)

  NGC, IC, UGC, Image Collection
NGC 1160 and NGC 1161, Galaxies in Perseus
NGC 6548, and NGC 6549, Galaxies in Hercules.
NGC 7778, 7779, 7780, 7781, 7782, and MCG 1-60-044, aka Galaxy Cluster Zwicky 2350.6+0758
www.kopernik.org /images/archive/ngcindex.htm   (4852 words)

 NGC 185
A first photograph of NGC 185 was obtained by James Edward Keeler with the Crossley Reflector of Lick Observatory between 1898 and 1900.
NGC 185 was recognized as a Local Group member galaxy, together with its neighbor NGC 147, by Walter Baade (1944), when he resolved them into stars with the 100-inch reflector on Mt. Wilson.
The Binary Galaxies NGC 147 and NGC 185.
www.seds.org /~spider/spider/LG/n0185.html   (421 words)

 Cosmic Voyage-The Online Resource for Amateur Astronomers   (Site not responding. Last check: 2007-10-08)
NGC 185 is a 9.2 magnitude satellite galaxy of the great Andromeda galaxy, M31.
It is located in Cassiopeia about 1 degrees east of NGC 147, another satellite of M31.
NGC 185 has a slightly higher surface brightness than nearby NGC 147--22.9 magnitudes per square arc second compared to 23.0 magnitudes per square arc second--which makes for a somewhat better view.
hometown.aol.com /billferris/n185.html   (125 words)

 NGC 147 - Wikipedia, the free encyclopedia
NGC 147 is a Dwarf spheroidal galaxy about 2.7 million light-years away in the constellation Cassiopeia.
NGC is a member of the Local group of galaxies and a satellite galaxy of the Andromeda Galaxy (M31).
The membership of NGC 147 in the Local Group was confirmed by Walter Baade in 1944 when he was able to resolve the galaxy into individual stars with the 100 inch telescope at Mount Wilson near Los Angeles.
en.wikipedia.org /wiki/NGC_147   (294 words)

 Local Group
NGC 404 - Elliptical or Lenticular Galaxy (E0 or SA(s)0- in Andromeda
NGC 1569 - Irregular Galaxy (Irp+ III-IV) in Camelopardalis
NGC 1560 (IC 2062) - Spiral Galaxy (Sd) in Camelopardalis
www.ebroadcast.com.au /lookup/encyclopedia/lo/Local_Group.html   (586 words)

 NGC 185 - Wikipedia, the free encyclopedia
NGC 185 is a dwarf elliptical galaxy about 2.08 million light-years away in the constellation Cassiopeia.
NGC 185 is a satellite galaxy of the famous Andromeda Galaxy (M31) and was discovered by William Herschel on November 30, 1787.
Unlike most dwarf elleptical galaxies, NGC 185 actually contains young stellar clusters and star formation proceeded at a low rate until the recent past.
en.wikipedia.org /wiki/NGC_185   (131 words)

 Doug's Deep Sky Challenge - Astronomical Companions.
NGC 5195, at magnitude 9.6, is easily seen just a few arc minutes to the north of its spectacular face-on spiral parent.
M32, or NGC 221, is an elliptical galaxy that shines at magnitude 8.1.
NGCs 147 and 185 lie about seven degrees to the north, so most observers don’t realize that they are gravitationally bound companions to M31.
www.umich.edu /~lowbrows/reflections/2006/dscobel.23.html   (1174 words)

 IngentaConnect The internal dynamics of the Local Group dwarf elliptical galaxie...   (Site not responding. Last check: 2007-10-08)
For NGC 185, having a much rounder appearance on the sky, we produced models for different inclinations.
NGC 205 and 147 have a relatively isotropic velocity dispersion tensor within the region where the internal dynamics are strongly constrained by the data.
Our estimated inclination for NGC 185 is i≈ 50° because in that case the model has an intrinsic flattening close to the peak of the intrinsic shape distribution of dEs and it, like the best-fitting models for NGC 147 and 205, is nearly isotropic.
www.ingentaconnect.com /content/bsc/mnr/2006/00000369/00000003/art00027   (401 words)

 Ole's Astronomy Site: Galaxies in the Andromeda Subgroup
The large red object to the upper left is NGC 604, one of the largest H-II regions known.
NGC 147 is a satellite galaxy of M31 and located somewhat closer to us than the Andromeda Galaxy.
It is a dwarf elliptical galaxy similar to NGC 205 (M110).
www.ngc7000.org /ccd/gal-andromeda.html   (611 words)

 Seasonal Excerpt from The Deep Sky: An Introduction
NGC 7789 is famous for being one of the densest open clusters north of the celestial equator.
NGC 147 and NGC 185, mentioned earlier as two of the Andromeda Galaxy's companion systems, are found within 1° of each other, but about 7° north of M31 over the border in Cassiopeia.
NGC 185, found about 1° due west of Omicron, is the easier of the pair to spot.
www.philharrington.net /dsexpt.htm   (2387 words)

 [No title]
NGC 185 was a faint 3 x 2 arcmin oval with no sharp center and a gradual fade out to nothing from the center.
Luckily, NGC 2169 was quite interesting, with 17 stars in clumps and with a general parallelogram shape and bright corners.
I made it to NGC 2264 and could imagine that only part of the overall rich star pattern was part of the cluster, but could not see any hint of nebulosity just 35 degrees above the cities.
www.eskimo.com /~rachford/observing/reports/obs_20030102.txt   (785 words)

 Structures of the Dwarf Elliptical Galaxies NGC 185 and NGC 205 (ResearchIndex)
Structures of the Dwarf Elliptical Galaxies NGC 185 and NGC 205 (ResearchIndex)
Structures of the Dwarf Elliptical Galaxies NGC 185 and NGC 205
Abstract: INTRODUCTION NGC 185 and NGC 205, companions of M31, are dwarf elliptical galaxies with peculiar features such as distinguishable dust clouds and bright blue stars.
citeseer.ist.psu.edu /487686.html   (233 words)

 NGC 185, a dwarf elliptical galaxy   (Site not responding. Last check: 2007-10-08)
This image of dwarf elliptical galaxy NGC 185 is a 10 minute exposure with an ST-6 CCD camera thru a 20 inch F/8.1 telescope.
(referring to NGCs 147 and 185) These two miniature elliptical galaxies appear to be distant companions of the Great Andromeda Galaxy M31.
NGC 185 is the brighter of the two, and may be seen in a good 6 inch telescope......
www.kopernik.org /images/archive/n185.htm   (176 words)

 21st  December 1999   (Site not responding. Last check: 2007-10-08)
The observation of recent star formation in the galaxy NGC 187 contradicts the scheme established in the 1940s by the distinguished astronomer Walter Baade according to which dwarf elliptical galaxies are populated only by old stars.
Researchers at the IAC began to study NGC 185 in 1996, using the Jakobus Kapteyn Telescope (JKT) and Nordic Optical Telescope (NOT) at the Roque de los Muchachos Observatory.
On the other hand, adds Aparicio, ‘the stellar clusters we have found are a trace of the last star formation episode that occurred in NGC 185, hundreds of millions of years ago (in comparison, the age of the galaxy and its oldest stars is some 10 000 to 15 000 million years).
www.iac.es /gabinete/noticias/1999/21dic1.htm   (840 words)

 Deep gems in an autumn night   (Site not responding. Last check: 2007-10-08)
NGC 246, a Planetary Nebula in Cetus by Peter Natscher
Begin with NGC 40, a beautiful and interesting planetary nebula in Cassiopeia (RA 00.13.09 Dec +72 31 20).
NGC 185 is a large dim galaxy, a satellite of M31.
ephemeris.sjaa.net /0310/e.html   (767 words)

Galaxy M 31 - NGC 224 (the Great Andromeda Galaxy, formerly the Great Andromeda Nebula) is the nearest big spiral galaxy, the member of the Local Group of galaxies.
There are four satellite galaxies in its proximity, viz., M 32 - NGC 221, situated 0.4 deg to the south, M 110 - NGC 205, situated 0.6 deg to NW, and NGC 185 and NGC 147, situated in Cassiopeia.
M 31 can be seen by the naked eye as an elongated misty cloud, which has a diameter of 3 deg and over in binoculars.
www.avastronomyclub.org /const/and.htm   (244 words)

 SPACE.com -- Hubble Unveils Double Star Cluster in Nearby Galaxy
NGC 185 is an unusual double star cluster lying in the Large Magellanic Cloud, a satellite galaxy of the Milky Way.
A filamentary nebula that surrounds NGC 1850 is evidence of this supernova.
The formation piqued the interest of STScI scientists because the stars surrounding NGC 1850 are a billion years old.
www.space.com /scienceastronomy/astronomy/hubble_cluster_010710.html   (752 words)

 [No title]
I bagged 4 new ones, but none of the observations were particularly good due to the deteriorating conditions and their southerly locations.
NGC 157 was a faint oval about 3 by 2 arcmin with no bright core.
I had tried NGC 247 last night within the Denver light dome and was unsuccessful.
www.eskimo.com /~rachford/observing/reports/obs_20021207.txt   (823 words)

 NGC 185 concept from the Astronomy knowledge base
NGC 185 concept from the Astronomy knowledge base
physical object > natural object > celestial body > collection of stars > galaxy > elliptical galaxy > dwarf elliptical galaxy > NGC 185
Next dwarf elliptical galaxy: Leo dwarf Up: dwarf elliptical galaxy Previous dwarf elliptical galaxy: NGC 147
www.site.uottawa.ca:4321 /astronomy/NGC185.html   (57 words)

 NGC Gallery
There are numerous images of NGC, IC, and a few minor catalogue objects scattered around the other Gallery pages, taken with various instruments and interspersed with text.
NGC 2024 again, this time with the Artemis 285 and TMB refractor., also including B33, the Horsehead nebula.
NGC 6543 - the Cat's Eye Nebula in Draco.
mysite.wanadoo-members.co.uk /astroplover/NGC.htm   (136 words)

 SW: Deep Andromeda - Satellite Galaxies, Star Clouds and Globular Clusters of M31 - Article
NGC 147 and NGC 185 lie some seven degrees away are often overlooked.
That honor goes to NGC 206, which is visible in small apertures if you know what you’re looking for.
NGC 206 is a giant star cloud located in the southwestern arm, large enough and bright enough for William Herschel to give it a separate catalog number following his observation of it in October of 1786.
cloudynights.com /item.php?item_id=1559   (2660 words)

 And - Andromeda
NGC: 0205, 0214, 0221, 0224, 0404, 0752, 0753, 0891, 7640, 7662, 7686,
Very bright and large, much elongated in position angle 165 degrees, very gradually brightening to a very much brigher middle.
Observers have sometimes recognized the star in a 350-mm.
mypage.bluewindow.ch /horo/ngc/and.htm   (412 words)

NGC 7789 160 Stars estimated by counting 40 in the N to W quadrant.
NGC 7789 in 10" with 12mm Nagler, estimated 120 stars resolved by counting 40 in the NW quadrant.
NGC 7789 with 27mm is stupendous, 75 stars in SW quadrant, four orange stars and 20 dark yellow.
www.saguaroastro.org /content/obsnotes/CASSIOPEIA.htm   (2500 words)

 Catalogue: J/A+A/403/93/ngc185
J/A+A/403/93 Photometry of AGB stars in NGC 185 and NGC 147 (Nowotny+, 2003) ================================================================================ A census of AGB stars in Local Group galaxies.
The major parts of two dwarf galaxies, NGC 185 and NGC 147, were observed; 154 new AGB carbon stars in NGC 185 and 146 in NGC 147 were identified.
This file × ngc185.dat 55 26496 Coordinates, chemistry flag and photometry of stars in NGC 185 × ngc147.dat 55 18300 Coordinates, chemistry flag and photometry of stars in NGC 147
vizier.u-strasbg.fr /cgi-bin/Cat?J/A+A/403/93/ngc185   (450 words)

 The Star-Forming ISM of Two Nearby Dwarf Elliptical Galaxies   (Site not responding. Last check: 2007-10-08)
We present a study of the components of the interstellar medium (ISM) in NGC 185 and NGC 205, two dwarf elliptical companions of M31.
HI in NGC 185, and to a lesser extent in NGC 205, can be separated into broad (\sigma \approx13 km/s) and narrow (\sigma \approx3 km/s) components with different distributions and kinematics.
Comparison with CO spectra shows that the variations in gas dispersion from place to place in the galaxies are mostly due to differing amounts of nonthermal or turbulent broadening in the ISM.
www.aas.org /publications/baas/v27n4/aas187/S011009.html   (264 words)

 HI distribution in extreme dIrr's & dE's
Before looking at the ISM in dSph galaxies, it is instructive to look at what is known on the HI distribution in low luminosity dE and dIrr galaxies.
For the dE's, the best study is the one of Young and Lo (1997a), where they looked at the HI content and distribution of NGC 185 and NGC 205.
NE for NGC 185) from the optical center.
www.atnf.csiro.au /pasa/16_1/carignan/paper/node2.html   (318 words)

 NGC-185   (Site not responding. Last check: 2007-10-08)
Not listed in Norton's Star Atlas, 185 was not even seen by Herschel.
Yet it was found fairly easily in my 6-inch scope in the lower regions of Cassiopeia.
Nearby is NGC-145, a similar local member, but one I have been unable to find to date.
clifty.com /scott/DSO/185.html   (84 words)

 Catalog of NGC Images
The following links access a wide variety of NGC Catalog deep space objects.
Many of these images are copyrighted and must not be copied into your machines without permission of the owner.
Some of these images are quite large and may take a long time to transmit.
www.frostydrew.org /transfer/fullngc.htm   (60 words)

 [No title]
# NGC objects: # This is data from the SAGUARO ASTRONOMY CLUB DATABASE, VERSION 6.0, updated # with the Third Catalog of Bright Galaxies.
# N.B.: dark nebulae are assigned a magnitude of 10.98, # N.B.: NGC 292 had SMC added by hand.
# N.B.: NGC objects which correspond to Messier objects have been commented out.
spiff.rit.edu /classes/phys445/catalogs/NGC.edb   (70 words)

 Extragalactic Novae - 2003.
Located 185" east and 282" south of the center of NGC 224 (= M31) (Marco Fiaschi image)
Located 36".2 west and 7".6 north of the center of NGC 224 (= M31) (Kamil Hornoch discovery image) (Marco Fiaschi discovery image)
Mag 18.5*, Type variable star (this is a galactic object) (References:
www.rochesterastronomy.org /sn2003/novae.html   (840 words)

 10-8-05 - Astronomy.com Forums
Objects Observed- NGC 185, NGC 127, M33 and HII regions, NGC 404
This is what I think happened with N 185.
Yup that looks like NGC 185 to me. At least the view of it through my 6" scope.
www.astronomy.com /ASY/CS/forums/290143/ShowPost.aspx   (709 words)

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