Antawaqalla ñuñuwarani
Antawaqalla ñuñuwarani | |
---|---|
Observation data (J2000 epoch) | |
Constellation | Sculptor |
Right ascension | 00h 37m 41.1s[2] |
Declination | −33° 42′ 59″[2] |
Redshift | 9050 ± 3 km/s[2] |
Distance | 500 Mly (150 Mpc)[3] |
Apparent magnitude (V) | 15.2[2] |
Characteristics | |
Type | S pec (Ring)[2] |
Size | 44.23 kpc (144,300 ly) (diameter; 25.0 mag/arcsec2 B-band isophote)[2][4] |
Apparent size (V) | 1′.1 × 0′.9[2] |
Notable features | Ring shape |
Other designations | |
MCG-06-02-022a,[2] PGC 2248[2] |
Antawaqalla ñuñu warani (ESO 350-40 icha PGC 2248 nisqapas) nisqaqa huk lenticular anillu ñuñuwaranim, yaqa 500 hunu k'anchay wata karum Sculptor hawa phuyu huñupi.[1] D 25 isofotal diámetro 44.23 kiloparsec (144,300 wata k'ancha), yaqa 2.9–4.8 × 109 inti masayuq masayuq; hawa anillunqa 217 km/s muyuriq rit'iyuq.[5]
Fritz Zwicky sutiyuq runam 1941 watapi tarirqan [6] Zwickyqa tarisqantaqa "quyllurkunap dinámica nisqapi sut'inchayninta suyaq aswan sasachakuyniyuq estructurakunamanta hukninmi" nispam qhawarirqan.[7][8]
Chay ñuñuwarani nisqap hatun kayninmanta yupayqa 150.000 k'anchay watatam tukuchirqan, Andrómeda ñuñuwarani nisqamanta aswan huch'uylla.[9] Kimsa kaq Catálogo de Referencia de Galaxias brillantes (RC3) tupurqa D 25 isofotal diámetro nisqatam antawaqalla ñuñuwarani nisqapaq yaqa 60,9 arcosegundos nisqapi,[4] 44.23 kiloparsec (144,300 k'ancha-wata) diámetro nisqatam qurqan, 132.2 megaparsec (431 hunu k'ancha-wata) puka desplazamientomanta hurqusqa karumanta.[10]
Hatun antawaqalla ñuñuwarani nisqaqa Antawaqalla ñuñuwarani nisqa huñupi kamachiqmi, tawa aychapi tinkisqa espiral galaxiakunamantam. Chay kimsa compañeros nisqakunatam achka estudiokunapi sutichanku G1 nispa, aswan uchuy irregular azul espiral Magallanica nisqa; G2, q’illu compacto espiral nisqa, marea chupayuq; hinaspa G3, aswan karu espiral sapa kuti rikusqa ancho campo siq’ikunapi.
SN 2021afdx, Antawaqalla ñuñuwaranipi iskay rikch'aq hatun qucha, 2021 watapi inti raymi killapi tarisqa.[11][12]
X-wach'i hurqusqakuna
[llamk'apuy | pukyuta llamk'apuy]Pukyukuna
[llamk'apuy | pukyuta llamk'apuy]- ↑ 1,0 1,1 Marks, Anastasia (4 August 2022). "The Cartwheel Galaxy Is the Webb Telescope's Latest Cosmic Snapshot - Scientists gained new insights into the distant object, which got its distinctive shape from a collision with another galaxy". The New York Times. Retrieved 4 August 2022. Pukyumanta willaypi pantasqa: Etiqueta
<ref>
no válida; el nombre «NYT-20220804» está definido varias veces con contenidos diferentes - ↑ 2,0 2,1 2,2 2,3 2,4 2,5 2,6 2,7 2,8 La página Módulo:Citation/CS1/styles.css no contiene nada."NASA/IPAC Extragalactic Database". Results for Cartwheel Galaxy. Retrieved 2006-11-25.
- ↑ La página Módulo:Citation/CS1/styles.css no contiene nada.Moore, Patrick (2000). The Data Book of Astronomy. CRC Press. p. 318. ISBN 0-7503-0620-3.
- ↑ 4,0 4,1 La página Módulo:Citation/CS1/styles.css no contiene nada.De Vaucouleurs, Gerard; De Vaucouleurs, Antoinette; Corwin, Herold G.; Buta, Ronald J.; Paturel, Georges; Fouque, Pascal (1991). Third Reference Catalogue of Bright Galaxies. Bibcode:1991rc3..book.....D.
- ↑ "The Hα kinematic of the Cartwheel galaxy". Astron. Astrophys. 330: 881–93. February 1998. Bibcode 1998A&A...330..881A.
- ↑ Zwicky F (1941). in Theodore van Karman Anniversary volume Contribution to Applied Mechanics and Related Subjects. Pasadena, California: California Institute of Technology. p. 137.
- ↑ Zwicky F (1941). in Theodore van Karman Anniversary volume Contribution to Applied Mechanics and Related Subjects. Pasadena, California: California Institute of Technology. p. 137.
- ↑ Griv E (Oct 2005). "Origin of the Cartwheel Galaxy: disk instability?". Astrophys. Space Sci. 299 (4): 371–85. Error: Bad DOI specified. Bibcode 2005Ap&SS.299..371G.
- ↑ Amazing Space- Fast Facts: Cartwheel Galaxy. Amazing Space (2008)
- ↑ The Hα kinematic of the Cartwheel galaxy. 1998. https://ui.adsabs.harvard.edu/abs/1998A&A...330..881A/abstract.
- ↑ 2021afdx
- ↑ SN 2021afdx. IAU Supernova Working Group