Abell 1413#Abell 1413 BCG

Abell 1413 is one of the original 2,712 galaxy clusters compiled in the Abell catalogue, compiled by the American astronomer George O. Abell in 1958, using data retrieved from the National Geographic Society – Palomar Observatory Sky Survey.

Abell 1413 is classified as a type I galaxy cluster, characterized due to the presence of a single, massive galaxy in its center that dominates its smaller members. Thomas W. Noonan in 1971 characterized the cluster as having 60% the richness of the Coma Cluster, based on the assumption that the central cD elliptical is not a foreground object.{{Cite journal|url=https://ui.adsabs.harvard.edu/abs/1972AJ.....77....9N|title=The Cluster of Galaxies Abell 1413|first=Thomas W.|last=Noonan|date=February 1, 1972|journal=The Astronomical Journal|volume=77|page=9|via=NASA ADS|doi=10.1086/111237|bibcode=1972AJ.....77....9N }}

{{Infobox galaxy

| name = Abell 1413 Brightest Cluster Galaxy

| image = 300px

| caption = Detail of the supergiant elliptical galaxy Abell 1413 BCG, taken by the Chandra X-ray Observatory overlaid with optical wavelength data

| epoch = J2000

| constellation name = Leo

| ra = {{RA|11|55|18.00}}{{Cite web|url=https://ned.ipac.caltech.edu/byname?objname=ACO+1413&hconst=67.8&omegam=0.308&omegav=0.692&wmap=4&corr_z=1|title=By Name | NASA/IPAC Extragalactic Database|website=ned.ipac.caltech.edu}}

| dec = {{DEC|+23|24|17.81}}

| z = 0.14291

| h_radial_v = {{val|42843.95|100.13|u=km/s|fmt=commas}}

| gal_v = {{val|42811|100|u=km/s|fmt=commas}}

| dist_pc = {{cvt|0|+/-|637.45|Mpc|e9ly|0|lk=on}}{{hub|0.678}}

| group_cluster = Abell 1413

| type = E; BrClG

| size = {{convert|245.71|kpc|ly|sigfig=3|abbr=on|lk=on}}
(diameter; 25.0 mag/arcsec² r-band isophote (SDSS)

| appmag_v = 17.82

| names = MCG +04-28-097; WISEA J115518.00+232418.2; 2MASX J11551798+2324177; OGC 32; PGC 37477; Abell 1413 A

}}

The brightest cluster galaxy of Abell 1413, or Abell 1413 BCG (MCG 04-28-097) is the supergiant elliptical galaxy that is the dominant member of the cluster. As early as 1965, astronomers William Wilson Morgan and Janet Rountree Lesh pointed out the galaxy's extreme nature, citing it as a "very large and luminous central galaxy" that could possibly be the largest of all cD ellipticals discovered, and hence must be checked for being a possible foreground object.{{cite journal | last1 = Morgan | first1 = W. W. | last2 = Rountree Lesh | first2 = Janet | title = The Supergiant Galaxies. | journal = The Astrophysical Journal | date = 1965 | volume = 142 | pages = 1364–1365 |doi = 10.1086/148422 | doi-access = free }}

During the following decade, several other papers observed the cluster, particularly its cD galaxy, hence revealing its very extreme properties. It was found to be among the most luminous galaxies known,{{cite journal |last1=Oemler Jr. |first1=A. |title=The Systematic Properties of Clusters of Galaxies. Photometry of 15 Clusters |journal=Astrophysical Journal |date=November 1974 |volume=194 |page=20 |doi=10.1086/153216 |bibcode=1974ApJ...194....1O |url=https://ui.adsabs.harvard.edu/abs/1974ApJ...194....1O/abstract |access-date=18 March 2023|doi-access=free }}

{{cite journal |last1=Austin |first1=T.B. |last2=Peach |first2=J.V. |title=Studies of rich clusters of galaxies - II. The structure and luminosity function of the cluster A 1413. |journal=Monthly Notices of the Royal Astronomical Society |date=September 1974 |volume=168 |issue=3 |pages=591–602 |doi=10.1093/mnras/168.3.591 |bibcode=1974MNRAS.168..591A |url=https://ui.adsabs.harvard.edu/abs/1974MNRAS.168..591A/abstract |access-date=18 March 2023|doi-access=free }} and a titanic envelope was observed using very deep photographic plates.{{cite journal |last1=Oemler Jr. |first1=A.|title=The structure of elliptical and cD galaxies. |journal=Astrophysical Journal |date=November 1976 |volume=209 |page=17 |doi=10.1086/154769 |bibcode=1976ApJ...209..693O |url=https://ui.adsabs.harvard.edu/abs/1976ApJ...209..693O/abstract|doi-access=free }}{{cite journal |last1=Schombert |first1=James M. |title=The Structure of Brightest Cluster Members. III. cD Envelopes |journal=Astrophysical Journal |date=May 1988 |volume=328 |page=14 |doi=10.1086/166306 |url=https://ui.adsabs.harvard.edu/abs/1988ApJ...328..475S/abstract |access-date=23 March 2023}} Following studies would then publish extremely large effective radii for the central galaxy.{{cite journal |last1=Tonry |first1=John L. |title=Properties of CD galaxies. |journal=Proceedings of the 127th symposium of the IAU held in Princeton, U.S.A. |date=1987 |page=10 |doi=10.1007/978-94-009-3971-4_7 |url=https://ui.adsabs.harvard.edu/abs/1987IAUS..127...89T/abstract |access-date=20 March 2023}}{{cite journal |last1=Schombert |first1=James M. |title=The Structure of Brightest Cluster Members. II. Mergers |journal=Astrophysical Journal Supplement |date=August 1987 |volume=64 |page=24 |doi=10.1086/191212 |url=https://ui.adsabs.harvard.edu/abs/1987ApJS...64..643S/abstract |access-date=20 March 2023}}

Abell 1413 BCG is also notable due to its extreme ellipticity, making it the most elliptical brightest cluster galaxy known. It is rare for brightest cluster galaxies to have such an ellipticity; even then, Abell 1413 BCG is the most extreme known example of all of these.{{cite journal |last1=Porter |first1=Alain C. |last2=Schneider |first2=Donald P. |last3=Hoessel |first3=John G. |title=CCD Observations of Abell Clusters. V. Isophotometry of 175 Brightest Elliptical Galaxies in Abell Clusters |journal=Astrophysical Journal |date=May 1991 |volume=101 |page=35 |doi=10.1086/115788 |url=https://ui.adsabs.harvard.edu/abs/1991AJ....101.1561P/abstract |access-date=22 March 2023}}

Abell 1413 is located 2 billion light years away from Earth between the constellations of Leo and Coma Berenices.{{Cite news|url=https://scitechdaily.com/hubble-views-galaxy-cluster-abell-1413/|title=Hubble Views Galaxy Cluster Abell 1413|date=2014-11-10|work=SciTech Daily|access-date=2017-10-19|language=en-US}} 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.{{citation needed|date=October 2017}} 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. Scientists using the Canada-France-Hawaii telescope observed Abell 1413 and built a sample of over 250 galaxies. These scientists consider Abell 1413 to be relaxed even though it has a highly elliptical shape.{{Cite journal|last1=Castagné|first1=D.|last2=Soucail|first2=G.|last3=Pointecouteau|first3=E.|last4=Cappi|first4=A.|last5=Maurogordato|first5=S.|last6=Benoist|first6=C.|last7=Ferrari|first7=C.|title=Deep optical observations of the massive galaxy cluster Abell 1413|url=https://www.aanda.org/articles/aa/full_html/2012/12/aa16837-11/aa16837-11.html#T2|journal=Astronomy & Astrophysics|language=en|volume=548|pages=A18|doi=10.1051/0004-6361/201116837|issn=0004-6361|bibcode=2012A&A...548A..18C|year=2012|doi-access=free}} The scientists also concluded that the cluster ellipticity at large radii is around .8 while the cluster ellipticity at the center is about .35, and that the cluster is aligned in the North-South direction, a few degrees westward.

• List of Abell clusters

{{reflist}}

{{Sky|11|55|18.9|+|23|24|31|1934000000}}

{{Catalogs|Abell=1413}}

{{Galaxy}}

{{Coma Berenices}}

{{DEFAULTSORT:Abell clusters}}

1413

Category:Galaxy clusters

Category:Abell richness class 3

Category:Leo (constellation)

Category:Coma Berenices