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- W203535548 abstract "We present the results of the first XMM-Newton observation of the interacting type IIn 1995N. The X-ray flux has dropped at a value about an order of magnitude lower than that of a previous ASCA observation of January 1998. The X-ray spectrum shows statistically significant evidence for the presence of two distinct thermal components at different temperatures. From these temperatures we derive that the exponent of the ejecta density distribution is n = 6.4. Coordinated optical and infrared observations allow us to reconstruct the simultaneous infrared to X-ray flux distribution of SN 1995N. We find that, at ∼8 years after explosion, the direct X-ray thermal emission due to the wind/ejecta interaction is ∼ 5 times larger than the total reprocessed IR/optical flux." @default.
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- W203535548 date "2006-01-01" @default.
- W203535548 modified "2023-09-23" @default.
- W203535548 title "XMM-Newton and VLT observations of SN 1995N." @default.
- W203535548 hasPublicationYear "2006" @default.
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