NGC 6221

{{Short description|Galaxy in the constellation Ara}}

{{Infobox galaxy

| name = NGC 6221

| image = NGC 6221 hst 05479 606.png

| caption = NGC 6221 as seen through the Hubble Space Telescope

| epoch = J2000

| pronounce =

| constellation name = Ara

| ra = {{RA|16|52|46.1}}

| dec = {{DEC|-59|13|07}}

| z = {{val|0.004999|0.000017}}

| h_radial_v = {{val|1499|5|u=km/s}}

| gal_v = {{val|1390|7|u=km/s}}

| dist_pc =

| dist_ly =

| group_cluster =

| type = SB(s)bc

| mass =

| mass_light_ratio =

| size = 70,000 light years

| stars =

| appmag_v = 9.28

| absmag_v = −20.97

| size_v = 3.5{{prime}} × 2.5{{prime}}

| notes =

| names = ESO 138-3, AM 1648-590, IRAS16484-5908 and PGC 59175

| references = NASA/IPAC extragalactic datatbase, http://spider.seds.org/

}}

NGC 6221 (also known as PGC 59175) is a barred spiral galaxy located in the constellation Ara. In de Vaucouleurs' galaxy morphological classification scheme, it is classified as SB(s)bc and was discovered by British astronomer John Herschel on 3 May 1835.{{cite web|title=NGC 6221 (= PGC 59175)|url=http://cseligman.com/text/atlas/ngc62.htm#6221|website=cseligman|access-date=3 October 2015}} NGC 6221 is located at about 69 million light years from Earth.{{cite web|title=Object No. 1 - NGC 6221|url=http://ned.ipac.caltech.edu/cgi-bin/objsearch?objname=NGC+6221&extend=no&hconst=73&omegam=0.27&omegav=0.73&corr_z=1&out_csys=Equatorial&out_equinox=J2000.0&obj_sort=RA+or+Longitude&of=pre_text&zv_breaker=30000.0&list_limit=5&img_stamp=YES|website=NASA/IPAC extragalactic database|publisher=NASA/IPAC|access-date=3 October 2015}}{{cite web|title=Revised NGC Data for NGC 6221|url=http://spider.seds.org/ngc/revngcic.cgi?NGC6221|website=Seds|access-date=3 October 2015}}

Galaxy group information

NGC 6221 is part of galaxy group NGC 6221/15, which includes spiral galaxy NGC 6215 and three dwarf galaxies. Interactions between NGC 6221 and NGC 6215 form a {{nowrap|double-stranded bridge}} of neutral hydrogen gas over a projected distance of 100 kpc; Dwarf 3 of the three dwarf galaxies may have formed from the bridging gas.{{cite journal|title=Neutral Hydrogen Gas in Interacting Galaxies: The NGC 6221 / 6215 galaxy group|url=http://www.atnf.csiro.au/people/bkoribal/ngc6221/|journal=Monthly Notices of the Royal Astronomical Society|volume=348|issue=4|pages=202–210|access-date=17 December 2015|bibcode=2004MNRAS.348.1255K|last1=Koribalski|first1=Bärbel|last2=Dickey|first2=John M.|year=2005|doi=10.1111/j.1365-2966.2004.07444.x|doi-access=free |arxiv=astro-ph/0501190}}

Supernovae

Two supernovae have been observed in NGC 6221:

  • SN 1990W (type Ib/Ic, mag. 15) was discovered by Robert Evans on 16 August 1990.{{cite journal|bibcode=1990IAUC.5076....1E |title=Supernova 1990W in NGC 6221 |last1=Evans |first1=R. |last2=Sadler |first2=E. |last3=McNaught |first3=R. H. |journal=International Astronomical Union Circular |date=1990 |issue=5076 |page=1 }}{{cite simbad|title=SN 1990W|accessdate=2021-03-19}}{{cite web | website=Transient Name Server | title=SN{{nbsp}}1990W | url=https://www.wis-tns.org/object/1990W | publisher = IAU | access-date=6 December 2024}}
  • SN 2024pxg (type II, mag. 15.1) was discovered by the Distance Less Than 40 Mpc Survey (DLT40) on 23 July 2024.{{cite web | website=Transient Name Server | title=SN{{nbsp}}2024pxg

| url=https://www.wis-tns.org/object/2024pxg | publisher = IAU | access-date=6 December 2024}}

See also

References

{{reflist}}