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The cluster lies at a distance of 10,000 light years from Earth and has an apparent magnitude of 7.4. Available Resources for NGC 2608 - Spiral Galaxy The higher the magnitude of an object, the fainter it appears. IV. It spans about 30,000 light years, lies about 68 million light years from Earth and can be seen with a small telescope in the constellation of Ursa Major. Apparent size 0.85 by 0.35 arcmin. – Object type: Open cluster. – Coordinates: RA: … 3. Visual magnitude and apparent dimension (arc min unless indicated as arc sec) Remarks NGC 6804 is above the horizon from Greenwich, United Kingdom . Some of the populations are found to belocated beyond the Perseus arm and may be the part of the Norma-Cygnus(outer) arm. A variable star periodically triples its light output. For example, Sirius has a magnitude of –1.46, while the brightest planet, Venus, can reach magnitude –4.9 at its brightest. M31 is best viewed during winter, is magnitude 4.5 *, and can be viewed with naked eye. This is the interactive NGC (and IC, and Messier) catalog at SEDS, based on the famous NGC 2000.0 by R.W. The DAY-I catalogue Context: We present the basic ideas and first results from the projectwe are carrying out at present, the search for and characterisation ofpre-main sequence (PMS) stars among the members of Galactic youngclusters. Pre-main sequence stars in open clusters. Only 35' to the southwest is the dauntingly dim object called the Bubble Nebula (NGC 7635), an even fainter ring of gas, whose brightest section abuts a 9th-magnitude star. Stars. See also rise and set times. We present colour-magnitude diagrams of open clusters, located in therange 112° l : 252°, manifesting stellar populations inthe background of clusters. Dreyer over 100 years ago. M66 lies at an estimated distance of 35 million light years. The Interactive NGC Catalog Online by Hartmut Frommert. The NGC/IC objects can be toggled on and off via the Display menu or palette. NGC 5248: m = 10.97. But actually NGC 6993 is a bright Sc galaxy (13.8 mag) in Capricornus.. IC 252 - Sinnott does not identify the object (type "blank"), but actually this is a pretty bright double galaxy with a total magnitude of 15.5 mag, located in Cetus. How much brighter is a magnitude +2 star than a magnitude +4 star? Messier 46. Messier 66 or M66 (also designated NGC 3627) is a spiral galaxywith an apparent visual magnitude of 8.9 and an angular diameter is 8x2.5 arc-minutes. By how much does the apparent magnitude change? The population in the background of open clusters: tracer of the Norma-Cygnus arm We present colour-magnitude diagrams of open clusters, located in therange 112° l 252°, manifesting stellar populations inthe background of clusters.Some of the populations are found to belocated beyond the Perseus arm and may be the part of the Norma-Cygnus(outer) arm. Sinnott of Sky Publishing Corp., who also created the electronic version used by this online service (thanks to Sky Publishing for permitting us this kind of use). NGC 7331 is the brightest member of the NGC 7331 Group of galaxies. Messier 29 is too faint to be spotted by the naked eye, but can be seen in binoculars. Answers: 1. NGC/IC Options ... Limit by Magnitude Criteria: If checked will use the settings from the magnitude dialog box. Given its visual magnitude of 12, NGC 6804 is visible with the help of a telescope havng an aperture of 8 inches (200mm) or more. dark nebulae) are also listed. Together with M65 and NGC 3628, the three galaxies are referred to as the Leo Triplet or the Trio in Leo. The 1,165 NGC objects in the NexStar 60/76/80/102/114/4/130 GT hand control database, including Dreyer's descriptions. NGC 5774-75: 14h54m00s +03°33' Virgo If unchecked, all the objects will be displayed irrespective of brightness. For reference, the full moon is 30' (arc minutes) in size. The absolute magnitude of the variablewas determined from the period-luminosity (P-L) relation for Galacticδ Scuti stars and from theoretical modeling of the observed B,V,Ilight curves with nonlinear pulsation models. Above, a 9 arcmin wide DSS image centered on NGC 2218 NGC 2219 3. I. Typical of reflection nebulae, they appear bluish resulting from light reflection from hot young stars by the interstellar dust, with darker regions dividing the three NGC objects. Messier object M51 (NGC 5194), also known as the Whirlpool Galaxy, is a spiral galaxy located in the constellation Ursa Major in the M51 Group of galaxies. II. Given its B magnitude of 13.2, NGC 2608 is visible with the help of a telescope havng an aperture of 10 inches (250mm) or more. The Equinox 2000 coordinates are RA= 11h 20.2m, Dec= +12° 59´. 2. The resultant colour-magnitude diagrams indicate that thecluster is an intermediate-age object of 1.4 Gyr. NGC 7331, also known as Caldwell 30, is an unbarred spiral galaxy located at around 40 million light-years away from us. The RASC's Finest N.G.C. The New General Catalog (NGC) is a listing of nearly 8,000 non-stellar objects, such as star clusters, nebulae, and galaxies, compiled by J.L.E. See also rise and set times. This grouping is positioned half a degree northeast of the great nebula. For reference, the … – Magnitude: +3 – Distance: About 1,321 light years – Other designations: C 1104-584, Caldwell 91, Melotte 103, Football Cluster, Wishing Well Cluster. The spiral arms of M66 appear deformed due to the gravitational effec… "Best" objects are marked in bold. Effects of metallicity, star-formation conditions, and evolution in B and Be stars. It has the designation NGC 6913 in the New General Catalogue. Messier 46, also designated as NGC 2437, is an open cluster that was discovered in 1771 by famous astronomer Charles Messier. NGC 5897 is a globular cluster in Libra with a low surface brightness, making it a more challenging object than its magnitude (8.5) would suggest. It has an apparent magnitude of 10.4. In thispaper we analyze the STEPSS observations of the open cluster NGC 1245 todetermine the variable-star content of the cluster. NGC 5350 Group: 13h53m24s +40°22' Canes Venatici: This group is positioned near a 6.5 magnitude star and has a bright spiral galaxy, NGC 5471 less than a half degree to the northeast. Overall it shines at magnitude … M51 is best viewed during early spring, is magnitude 8.0*, and can be viewed with binoculars.It is 11 x 7' in size. Only some minor corrections have been included in our online database. – Constellation: Canis Major. M101, M87, NGC 5248, NGC 4085, IC1410. Messier Objects Located in the Constellation of Puppis. Objects without magnitude (i.e. Some objects originally thought to be deep sky objects and listed in the NGC have been subsequently shown to be ordinary stars, so their inclusion in the catalog is now considered erroneous. Objects are sorted by catalog number, starting with Messier list, then NGC, IC and so on. All structured data from the file and property namespaces is available under the Creative Commons CC0 License; all unstructured text is available under the Creative Commons Attribution-ShareAlike License; additional terms may apply. The Messier objects are a set of 110 astronomical objects catalogued by the French astronomer Charles Messier in his Catalogue des Nébuleuses et des Amas d'Étoiles ("Catalogue of Nebulae and Star Clusters"). There are 3 Messier Objects located in the constellation of Puppis, namely the Messier 46, Messier 47, and Messier 93 open clusters. Physical Information: The asterism consists of five 14th to 15th magnitude stars arranged in a north-south oval, and a few much fainter stars that Cooper could not have seen; so the NGC object is basically just the five brighter stars. I have therefore looked at the range of magnitudes in different wavelength ranges in several references, and at the visual magnitude estimates in Steve Gottlieb's visual examination of the NGC/IC objects. This list of stars is based on the 'NGC 2000.0' version of the catalog, which lists the stars in its errata, supplemented with data on each individual star from the VizieR database. It lies about 5,400 light years from Earth in the direction of Puppis constellation. This spiral galaxy was discovered by Messier in 1780. Small Magellanic Cloud, field of NGC 330 Aims.We search for the effects of metallicity on B and Be stars in theSmall and Large Magellanic Clouds (SMC and LMC) and in the Milky Way(MW), by extending our previous analysis of B and Be star populations inthe LMC to the SMC. - spiral galaxy was discovered by Messier in 1780 populations inthe background of clusters while the brightest planet Venus! Estimated distance of 4,000 light years from Earth observed in telescopes at the lowest powers box! Arms of m66 appear deformed due to the gravitational effec… the higher the of. As the Leo Triplet or the Trio in Leo ngc objects by magnitude ) is an open with... Cluster located in the direction of Puppis constellation page was last edited on 8 February 2011, at 20:40 with. And another with a blue horizontal branch and another with a blue horizontal branch 2000 coordinates are 11h! Overall it shines at magnitude … the NGC/IC objects can be toggled on and off via the Display or. 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