Academic Journal

The Highest Redshift Relativistic Jets

التفاصيل البيبلوغرافية
العنوان: The Highest Redshift Relativistic Jets
المؤلفون: C. C. Cheung, A. Siemiginowska, D. E Harris, D. A. Schwartz, J. F. C. Wardle, D. Gobeille, N. P. Lee
المساهمون: The Pennsylvania State University CiteSeerX Archives
المصدر: http://www.slac.stanford.edu/pubs/slacpubs/13000/slac-pub-13055.pdf.
سنة النشر: 2007
المجموعة: CiteSeerX
الوصف: We describe our efforts to understand large-scale (10’s–100’s kpc) relativistic jet systems through observations of the highest-redshift quasars. Results from a VLA survey search for radio jets in ∼30 z>3.4 quasars are described along with new Chandra observations of 4 selected targets. 1. Why High-redshift Jets? It is now well established that X-ray emission is a common feature of kiloparsecscale radio jets (see Harris & Krawczynski 2006, for a recent review and the associated website
نوع الوثيقة: text
وصف الملف: application/pdf
اللغة: English
Relation: http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.409.8567; http://www.slac.stanford.edu/pubs/slacpubs/13000/slac-pub-13055.pdf
الاتاحة: http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.409.8567
http://www.slac.stanford.edu/pubs/slacpubs/13000/slac-pub-13055.pdf
Rights: Metadata may be used without restrictions as long as the oai identifier remains attached to it.
رقم الانضمام: edsbas.7406FF5
قاعدة البيانات: BASE