The list is limited to declination -60°. Dreyer over 100 years ago. NGC 5248: m = 10.97. 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. We present colour-magnitude diagrams of open clusters, located in therange 112° l : 252°, manifesting stellar populations inthe background of clusters. 3. NGC 5774-75: 14h54m00s +03°33' Virgo This grouping is positioned half a degree northeast of the great nebula. astronomical catalogue of deep sky objects Spiral Galaxy NGC 3982 displays numerous spiral arms filled with bright stars, blue star clusters, and dark dust lanes. This is the interactive NGC (and IC, and Messier) catalog at SEDS, based on the famous NGC 2000.0 by R.W. Messier 29 is too faint to be spotted by the naked eye, but can be seen in binoculars. 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. 6.31 times brighter. 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. Its current altitude is 42° above the horizon. This page was last edited on 8 February 2011, at 20:40. dark nebulae) are also listed. It is 178' in size. – Coordinates: RA: … Messier 46 (NGC 2437) is an open cluster with an apparent magnitude of 6.5. 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. NGC/IC Options ... Limit by Magnitude Criteria: If checked will use the settings from the magnitude dialog box. The Interactive NGC Catalog Online by Hartmut Frommert. 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. See also rise and set times. NGC 7331 is the brightest member of the NGC 7331 Group of galaxies. 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. It is best observed in telescopes at the lowest powers. I. 3. – Object type: Open cluster. Messier 46, also designated as NGC 2437, is an open cluster that was discovered in 1771 by famous astronomer Charles Messier. 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. Messier 47 (M47) Messier 47 (NGC 2422) is an open cluster in Puppis. If unchecked, all the objects will be displayed irrespective of brightness. This spiral galaxy was discovered by Messier in 1780. Messier 46. 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. Available Resources for NGC 2608 - Spiral Galaxy 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. 2. The NGC/IC objects can be toggled on and off via the Display menu or palette. Only some minor corrections have been included in our online database. 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. 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. IV. Apparent size 0.85 by 0.35 arcmin. 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). "Best" objects are marked in bold. Above, a 9 arcmin wide DSS image centered on NGC 2218 NGC 2219 It has an apparent magnitude of 10.4. Globular clusters with composite color-magnitude diagrams, such as NGC1851, NGC 2808, and Fornax 3, might have formed by mergers. NGC 7331 was discovered in 1784 by the famous astronomer, William Herschel. Answers: 1. M51 is best viewed during early spring, is magnitude 8.0*, and can be viewed with binoculars.It is 11 x 7' in size. Caroline’s Cluster. NGC 7331, also known as Caldwell 30, is an unbarred spiral galaxy located at around 40 million light-years away from us. 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. Ngc 5248, NGC 4085, IC1410 spiral galaxy located at around 40 million light-years away from.. Positioned half a degree northeast of the NGC 7331 was discovered in 1784 the... Only some minor corrections have been included in our Online database we present diagrams! Is too faint to be spotted by the naked eye, but can be seen in.! 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