ブラックホール候補のXTE J1118+48080における相関した高速X線と光学的変動
G Kanbach1, C Straubmeier, H C Spruit
1Max-Planck-Institut für Extraterrestrische Physik, Postfach 1317, 85741 Garching, Germany.
Nature
|November 9, 2001
まとめ
ブラックホールの蓄積は,新しいX線と光学データにより,よりよく理解されています. XTE J1118+480の観測により,光学的光はサイクロシンクロトロン放出から発生し,放出が遅いことを示唆している.
科学分野:
- 天体物理学 天体物理学
- 高エネルギー天体物理学
- ブラックホールの蓄積物理学 ブラックホールの蓄積物理学
背景:
- ブラックホールは,恒星の伴星からのガス蓄積によって観測される.
- 標準的な薄型蓄積円盤モデルは,観測されたX線変動と流出を説明できていません.
研究 の 目的:
- ブラックホールの蓄積システムの物理的条件を調査するために.
- 暫定的な源におけるX線と光学的放射の間の謎めいた相関を説明するために.
主な方法:
- 高時間解像度のX線と光学的観測を同時に行う.
- 変速源XTE J1118+480.0.の解析について
主要な成果:
- 強い,謎めいたX線と光学放射の相関が観察されました.
- 光学放射はX線増量後に急激に上昇し,その後に低下した.
- 観測されたタイミングは,再処理されたX線放射モデルと矛盾しています.
結論:
- 光学放射は,ブラックホールの近くのサイクロシンクロトロン放射から発生している可能性が高い.
- 時間の依存性は,ゆっくり (<0.1c),磁気制御された流出を示唆しています.
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