+ Schneider + Clowe+, 2005 | Details on Acronym: [DSC2005] | |
[DSC2005] | ||
Write: | <<[DSC2005] A223-W>> <<[DSC2005] WW peak>> <<[DSC2005] arclet N>> | |
N: | 2+1+2 | |
Object: | ? (SIMBAD class: Unknown = Object of Unknown Nature) | |
Note: | Weak lensing analysis of the double cluster ACO 222 and ACO 223: ACO 223 shows two distinct peaks separated by about 4' in the galaxy distribution and X-ray emission. A223-N and A223-S. A new cluster is seen SE of ACO 222, designated as SE peak of galaxies. Two arclets are found in ACO 222. | |
in source: | ACO 222 | |
in source: | ACO 223 | |
Ref: | =2005A&A...440..453D | |
by | DIETRICH J.P. , SCHNEIDER P., CLOWE D., ROMANO-DIAZ E., KERP J. | |
Astron. Astrophys., 440, 453-471 (2005) | ||
Weak lensing study of dark matter filaments and application to the binary cluster A 222 and A 223. | ||
o | Text: <[DSC2005] A223-W> (Nos S, N). Text: <[DSC2005] SE peak> N=1. Table A1: <[DSC2005] arclet N> (Nos 1-2). | |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |