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Abell 1413 is a galaxy cluster in the Abell catalogue. The Abell catalogue was published by George O. Abell in 1958 while working on his PhD at California Institute of Technology[1]. The catalogue has two different surveys. The Northern survey was done first by Abell in 1958 with the help of A.G .Wilson. The Northern Survey had 2,712 clusters and in order for a cluster to be put into the catalogue it had to pass four criteria. The first was Richness, he divided the clusters into 6 different richness groups. Group 0 was 30-49 galaxies, Group 1 was 50-79 galaxies, Group 2 was 80-129 galaxies, Group 3 was 130 to 199 galaxies, Group 4 was 200-299 galaxies, and Group 5 was more than 299 galaxies. The second criteria was compactness .To pass this criteria a cluster must have 50 or more members in one counting radius of the clusters center. The third criteria is distance. A cluster must have a nominal redshift between .02 and .2, which means a recessional velocity is between 6,000 and 60,000 km/s. The fourth and final criteria was galactic latitude. Areas around the milky way were excluded because it was difficult to identify galaxy clusters[2]. The Southern survey was done in 1989 and added 1,361 clusters using the same criteria as the Northern Survey.
Abell 1413 is located 2 billion light years away from Earth between the constellations of Leo and Coma Berenices.[3] It is one of 4,073 clusters of galaxies at redshift (meaning they are moving away from earth,) that are somewhat close to the Earth[1]. Abell 1413 holds about 300 galaxies together with its strong gravity. Due to the strong interactions in the cluster, the material is heated up to 100 million degrees. Because of this intense heat, strong X-ray radiation is emitted from the cluster.[3] Scientists using the Canada-France-Hawaii telescope observed Abell 1413 and built a sample of over 250 galaxies. These scientist consider Abell 1413 relaxed even though it has a highly elliptical shape[4]. The scientist also concluded that the cluster ellipticity at large radii is around .35 while the cluster ellipticity at the center is about .8 and that the cluster is aligned in the North-South direction , a few degrees westward.[5]
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- ^ a b LLC, Revolvy,. ""Abell catalogue" on Revolvy.com". www.revolvy.com. Retrieved 2017-10-17.
{{cite web}}: CS1 maint: extra punctuation (link) CS1 maint: multiple names: authors list (link) - ^ LLC, Revolvy,. ""Abell catalog" on Revolvy.com". www.revolvy.com. Retrieved 2017-10-17.
{{cite web}}: CS1 maint: extra punctuation (link) CS1 maint: multiple names: authors list (link) - ^ a b "Hubble Views Galaxy Cluster Abell 1413". SciTech Daily. 2014-11-10. Retrieved 2017-10-15.
- ^ Castagné, D.; Soucail, G.; Pointecouteau, E.; Cappi, A.; Maurogordato, S.; Benoist, C.; Ferrari, C. (2012-12-01). "Deep optical observations of the massive galaxy cluster Abell 1413". Astronomy & Astrophysics. 548. doi:10.1051/0004-6361/201116837. ISSN 0004-6361.
{{cite journal}}: no-break space character in|title=at position 62 (help) - ^ Castagné, D.; Soucail, G.; Pointecouteau, E.; Cappi, A.; Maurogordato, S.; Benoist, C.; Ferrari, C. "Deep optical observations of the massive galaxy cluster Abell 1413". Astronomy & Astrophysics. 548. doi:10.1051/0004-6361/201116837. ISSN 0004-6361.
{{cite journal}}: no-break space character in|title=at position 62 (help)