Report
Intracluster light in clusters of galaxies at redshifts 0.4
التفاصيل البيبلوغرافية
العنوان:
Intracluster light in clusters of galaxies at redshifts 0.4
المؤلفون:
Guennou, L., Adami, C., Da Rocha, C., Durret, F., Ulmer, M. P., Allam, S., Basa, S., Benoist, C., Biviano, A., Clowe, D., Gavazzi, R., Halliday, C., Ilbert, O., Johnston, D., Just, D., Kron, R., Kubo, J. M., LeBrun, V., Marshall, P., Mazure, A., Murphy, K. J., Pereira, D. N. E., Rabaca, C. R., Rostagni, F., Rudnick, G., Russeil, D., Schrabback, T., Slezak, E., Tucker, D., Zaritsky, D.
سنة النشر:
2011
المجموعة:
Astrophysics
مصطلحات موضوعية:
Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics
الوصف:
The study of intracluster light can help us to understand the mechanisms taking place in galaxy clusters, and to place constraints on the cluster formation history and physical properties. However, owing to the intrinsic faintness of ICL emission, most searches and detailed studies of ICL have been limited to redshifts z<0.4.We search for ICL in a subsample of ten clusters detected by the ESO Distant Cluster Survey (EDisCS), at redshifts 0.4
نوع الوثيقة:
Working Paper
DOI:
10.1051/0004-6361/201117482
URL الوصول:
http://arxiv.org/abs/1109.3967
رقم الانضمام:
edsarx.1109.3967
قاعدة البيانات:
arXiv
| العنوان: | Intracluster light in clusters of galaxies at redshifts 0.4 |
|---|---|
| المؤلفون: | Guennou, L., Adami, C., Da Rocha, C., Durret, F., Ulmer, M. P., Allam, S., Basa, S., Benoist, C., Biviano, A., Clowe, D., Gavazzi, R., Halliday, C., Ilbert, O., Johnston, D., Just, D., Kron, R., Kubo, J. M., LeBrun, V., Marshall, P., Mazure, A., Murphy, K. J., Pereira, D. N. E., Rabaca, C. R., Rostagni, F., Rudnick, G., Russeil, D., Schrabback, T., Slezak, E., Tucker, D., Zaritsky, D. |
| سنة النشر: | 2011 |
| المجموعة: | Astrophysics |
| مصطلحات موضوعية: | Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics |
| الوصف: | The study of intracluster light can help us to understand the mechanisms taking place in galaxy clusters, and to place constraints on the cluster formation history and physical properties. However, owing to the intrinsic faintness of ICL emission, most searches and detailed studies of ICL have been limited to redshifts z<0.4.We search for ICL in a subsample of ten clusters detected by the ESO Distant Cluster Survey (EDisCS), at redshifts 0.4 |
| نوع الوثيقة: | Working Paper |
| DOI: | 10.1051/0004-6361/201117482 |
| URL الوصول: | http://arxiv.org/abs/1109.3967 |
| رقم الانضمام: | edsarx.1109.3967 |
| قاعدة البيانات: | arXiv |
| DOI: | 10.1051/0004-6361/201117482 |
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