Future instrumentation for the study of the warm-hot intergalactic medium

F. Paerels; J.S. Kaastra; T. Ohashi; P. Richter; A.M. Bykov; J. Nevalainen

Future instrumentation for the study of the warm-hot intergalactic medium

F. Paerels, J.S. Kaastra, T. Ohashi, P. Richter, A.M. Bykov, J. Nevalainen

Dept of Physics

extern

Research output: Contribution to journal › Article › Academic › peer-review

Abstract

We briefly review capabilities and requirements for future instrumentation in UV- and X-ray astronomy that can contribute to advancing our understanding of the diffuse, highly ionised intergalactic medium.

Original language	Undefined/Unknown
Pages (from-to)	405-418
Number of pages	14
Journal	Space Science Reviews
Volume	134
Issue number	1-4
Publication status	Published - 2008

Access to Document

Fulltext
Open Access (free)
Final published version, 364 KB

Cite this

@article{aade9d80878c424f8494c683eee1f826,

title = "Future instrumentation for the study of the warm-hot intergalactic medium",

abstract = "We briefly review capabilities and requirements for future instrumentation in UV- and X-ray astronomy that can contribute to advancing our understanding of the diffuse, highly ionised intergalactic medium.",

author = "F. Paerels and J.S. Kaastra and T. Ohashi and P. Richter and A.M. Bykov and J. Nevalainen",

year = "2008",

language = "Undefined/Unknown",

volume = "134",

pages = "405--418",

journal = "Space Science Reviews",

issn = "0038-6308",

publisher = "Springer Netherlands",

number = "1-4",

}

TY - JOUR

T1 - Future instrumentation for the study of the warm-hot intergalactic medium

AU - Paerels, F.

AU - Kaastra, J.S.

AU - Ohashi, T.

AU - Richter, P.

AU - Bykov, A.M.

AU - Nevalainen, J.

PY - 2008

Y1 - 2008

N2 - We briefly review capabilities and requirements for future instrumentation in UV- and X-ray astronomy that can contribute to advancing our understanding of the diffuse, highly ionised intergalactic medium.

AB - We briefly review capabilities and requirements for future instrumentation in UV- and X-ray astronomy that can contribute to advancing our understanding of the diffuse, highly ionised intergalactic medium.

M3 - Article

SN - 0038-6308

VL - 134

SP - 405

EP - 418

JO - Space Science Reviews

JF - Space Science Reviews

IS - 1-4

ER -