dc.contributor.author |
Verkhodanov, O. V. |
|
dc.contributor.author |
Khabibullina, M. L. |
|
dc.contributor.author |
Singh, M. |
|
dc.contributor.author |
Priya, A. |
|
dc.contributor.author |
Verkhodanova, N. V. |
|
dc.contributor.author |
Nandi, S. |
|
dc.date.accessioned |
2009-06-19T11:31:56Z |
|
dc.date.available |
2009-06-19T11:31:56Z |
|
dc.date.issued |
2008 |
|
dc.identifier.uri |
http://hdl.handle.net/123456789/50 |
|
dc.description.abstract |
Giant radio galaxies (GRGs) are considered as the largest single object in the Universe. They have sizes up to 12 Mpc. The reason of this is still unclear. However, several groups study these galaxies and explain the their properties by core-jet energy and environment. In this poster contribution, we describe our plans in the investigation of GRGs. We consider a problem of confusion of multipole ranges describing scales of GRGs and S-Z effects. Using the CATS data base, radio telescope RATAN-600 (SAO RAS) and Indian ARIES optical 101-cm telescope, the complex study of GRGs is suggested. |
en_US |
dc.language.iso |
en_US |
en_US |
dc.relation.ispartofseries |
Pr-Cosm2-247 |
|
dc.subject |
Radio Galaxies, cD Galaxies, N Galaxies |
en_US |
dc.title |
Giant radio galaxies: problems of understanding and problems for CMB? |
en_US |
dc.type |
Article |
en_US |