메뉴 건너뛰기




Volumn 401, Issue 1, 2003, Pages 197-203

XMM-Newton spectral analysis of the Pulsar Wind Nebula within the composite SNR G0.9+0.1

Author keywords

ISM: individual objects: G0.9+0.1; ISM: supernova remnants; X rays: ISM

Indexed keywords

ELECTRONS; SIGNAL TO NOISE RATIO; SPECTRUM ANALYSIS; WIND; X RAYS;

EID: 0037382867     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20021670     Document Type: Article
Times cited : (62)

References (24)
  • 8
    • 0012706736 scopus 로고    scopus 로고
    • Neutron Stars in Supernova Remnants, ed. P. O. Slane, & B. M. Gaensler
    • Gotthelf, E. V., & Olbert, C. M. 2002, in Neutron Stars in Supernova Remnants, ed. P. O. Slane, & B. M. Gaensler, ASP Conf. Proc., 271, 171
    • (2002) ASP Conf. Proc. , vol.271 , pp. 171
    • Gotthelf, E.V.1    Olbert, C.M.2
  • 9
    • 0003434576 scopus 로고    scopus 로고
    • Mullard Radio Astronomy Observatory, Cavendish Laboratory, Cambridge, United Kingdom
    • Green, D. A. 2001, A Catalogue of Galactic Supernova Remnants, Mullard Radio Astronomy Observatory, Cavendish Laboratory, Cambridge, United Kingdom (http://www.mrao.cam.ac.uk/surveys/snrs/).
    • (2001) A Catalogue of Galactic Supernova Remnants
    • Green, D.A.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.