dc.contributor.author | BALMAN, Şölen | |
dc.contributor.author | Pekon, Y. | |
dc.date.accessioned | 2021-03-06T10:24:17Z | |
dc.date.available | 2021-03-06T10:24:17Z | |
dc.identifier.citation | BALMAN Ş., Pekon Y., "High Resolution XMM-Newton Data of Nova Outbursts using Warm & Hot Absorber Models", 281st Symposium of the International-Astronomical-Union, Padova, İtalya, 4 - 08 Temmuz 2011, ss.124-125 | |
dc.identifier.other | av_ea32bc16-6fd9-47cf-8e60-0bb8ce50ee75 | |
dc.identifier.other | vv_1032021 | |
dc.identifier.uri | http://hdl.handle.net/20.500.12627/153838 | |
dc.identifier.uri | https://doi.org/10.1017/s1743921312014822 | |
dc.language.iso | eng | |
dc.subject | Temel Bilimler | |
dc.subject | Fizik | |
dc.subject | Astronomi ve Astrofizik | |
dc.subject | Temel Bilimler (SCI) | |
dc.subject | Uzay bilimi | |
dc.subject | ASTRONOMİ VE ASTROFİZİK | |
dc.title | High Resolution XMM-Newton Data of Nova Outbursts using Warm & Hot Absorber Models | |
dc.type | Bildiri | |
dc.contributor.department | Orta Doğu Teknik Üniversitesi , Fen Fakültesi , Astrofizik Ana Bilim Dalı | |
dc.contributor.firstauthorID | 2212701 | |