NGC 2237-9 & 2244 (Caldwell 49 & 50), Rosette Nebula and Cluster

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NGC 2237-9 & 2244 (Caldwell 49 & 50), Rosette Nebula and Cluster The Rosette Nebula (Caldwell 49) is a very large but dim emission nebula that surrounds an open cluster of young, blue-white stars. The cluster is NGC 2244 (also known as Caldwell 50 or the Rosette Cluster), and at magnitude 4.8 it is bright enough to be seen with binoculars or even the naked eye. The Rosette Nebula, however, has a low surface brightness, and although it is about twice the apparent diameter of the full Moon, it can be difficult to see except from a dark location. The nebula is about 5500 light years away. Find the Winter Hexagon, which is composed of six of the brightest stars in the sky-- Sirius, Procyon, Pollux, Capella, Aldebaran, and Rigel. On mid- winter evenings, these stars form a large oval stretching from low in the south to nearly overhead. As spring begins, the Winter Hexagon sinks toward the west. The constellation Orion and its bright red star Betelgeuse are inside the Hexagon. Start from bright red Betelgeuse, and look about 10 degrees to the east for a triangle of three dim (4th magnitude) stars, which are supposed to represent the head and neck area of Monoceros, the unicorn. As shown in the chart below, the Rosette Nebula and cluster are located within this triangle. At magnitude 4.8, the cluster should be easy to spot in binoculars. The large diffuse nebula around the cluster will be more difficult to see. Star hop from www.skyledge.net by Jim Mazur. Star charts created with Cartes du Ciel. .

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Rosette Nebula and Monoceros Loop
Oshkosh Scholar Page 43 Studying Complex Star-Forming Fields: Rosette Nebula and Monoceros Loop Chris Hathaway and Anthony Kuchera, co-authors Dr. Nadia Kaltcheva, Physics and Astronomy, faculty adviser Christopher Hathaway obtained a B.S. in physics in 2007 and is currently pursuing his masters in physics education at UW Oshkosh. He collaborated with Dr. Nadia Kaltcheva on his senior research project and presented their findings at theAmerican Astronomical Society meeting (2008), the Celebration of Scholarship at UW Oshkosh (2009), and the National Conference on Undergraduate Research in La Crosse, Wisconsin (2009). Anthony Kuchera graduated from UW Oshkosh in May 2008 with a B.S. in physics. He collaborated with Dr. Kaltcheva from fall 2006 through graduation. He presented his astronomy-related research at Posters in the Rotunda (2007 and 2008), the Wisconsin Space Conference (2007), the UW System Symposium for Undergraduate Research and Creative Activity (2007 and 2008), and the American Astronomical Society’s 211th meeting (2008). In December 2009 he earned an M.S. in physics from Florida State University where he is currently working toward a Ph.D. in experimental nuclear physics. Dr. Nadia Kaltcheva is a professor of physics and astronomy. She received her Ph.D. from the University of Sofia in Bulgaria. She joined the UW Oshkosh Physics and Astronomy Department in 2001. Her research interests are in the field of stellar photometry and its application to the study of Galactic star-forming fields and the spiral structure of the Milky Way. Abstract An investigation that presents a new analysis of the structure of the Northern Monoceros field was recently completed at the Department of Physics andAstronomy at UW Oshkosh.
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Spatial and Kinematic Structure of Monoceros Star-Forming Region
MNRAS 476, 3160–3168 (2018) doi:10.1093/mnras/sty447 Advance Access publication 2018 February 22 Spatial and kinematic structure of Monoceros star-forming region M. T. Costado1‹ and E. J. Alfaro2 1Departamento de Didactica,´ Universidad de Cadiz,´ E-11519 Puerto Real, Cadiz,´ Spain. Downloaded from https://academic.oup.com/mnras/article-abstract/476/3/3160/4898067 by Universidad de Granada - Biblioteca user on 13 April 2020 2Instituto de Astrof´ısica de Andaluc´ıa, CSIC, Apdo 3004, E-18080 Granada, Spain Accepted 2018 February 9. Received 2018 February 8; in original form 2017 December 14 ABSTRACT The principal aim of this work is to study the velocity ﬁeld in the Monoceros star-forming region using the radial velocity data available in the literature, as well as astrometric data from the Gaia ﬁrst release. This region is a large star-forming complex formed by two associations named Monoceros OB1 and OB2. We have collected radial velocity data for more than 400 stars in the area of 8 × 12 deg2 and distance for more than 200 objects. We apply a clustering analysis in the subspace of the phase space formed by angular coordinates and radial velocity or distance data using the Spectrum of Kinematic Grouping methodology. We found four and three spatial groupings in radial velocity and distance variables, respectively, corresponding to the Local arm, the central clusters forming the associations and the Perseus arm, respectively. Key words: techniques: radial velocities – astronomical data bases: miscellaneous – parallaxes – stars: formation – stars: kinematics and dynamics – open clusters and associations: general. Hoogerwerf & De Bruijne 1999;Lee&Chen2005; Lombardi, 1 INTRODUCTION Alves & Lada 2011).
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Winter Constellations
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Caldwell catalogue - Wikipedia, the free encyclopedia Log in / create account Article Discussion Read Edit View history Caldwell catalogue From Wikipedia, the free encyclopedia Main page Contents The Caldwell Catalogue is an astronomical catalog of 109 bright star clusters, nebulae, and galaxies for observation by amateur astronomers. The list was compiled Featured content by Sir Patrick Caldwell-Moore, better known as Patrick Moore, as a complement to the Messier Catalogue. Current events The Messier Catalogue is used frequently by amateur astronomers as a list of interesting deep-sky objects for observations, but Moore noted that the list did not include Random article many of the sky's brightest deep-sky objects, including the Hyades, the Double Cluster (NGC 869 and NGC 884), and NGC 253. Moreover, Moore observed that the Donate to Wikipedia Messier Catalogue, which was compiled based on observations in the Northern Hemisphere, excluded bright deep-sky objects visible in the Southern Hemisphere such [1][2] Interaction as Omega Centauri, Centaurus A, the Jewel Box, and 47 Tucanae. He quickly compiled a list of 109 objects (to match the number of objects in the Messier [3] Help Catalogue) and published it in Sky & Telescope in December 1995. About Wikipedia Since its publication, the catalogue has grown in popularity and usage within the amateur astronomical community. Small compilation errors in the original 1995 version Community portal of the list have since been corrected. Unusually, Moore used one of his surnames to name the list, and the catalogue adopts "C" numbers to rename objects with more Recent changes common designations.[4] Contact Wikipedia As stated above, the list was compiled from objects already identified by professional astronomers and commonly observed by amateur astronomers.
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