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2015 Fiscal Year Final Research Report

Search for black hole candidates deep within our Galaxy and understanding of their accretion processes through short-term X-ray variability study

Research Project

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Project/Area Number 24540239
Research Category

Grant-in-Aid for Scientific Research (C)

Allocation TypeMulti-year Fund
Section一般
Research Field Astronomy
Research InstitutionNihon University

Principal Investigator

NEGORO Hitoshi  日本大学, 理工学部, 教授 (30300891)

Research Collaborator FUKUSHIMA Kosuke  
SUZUKI Kazuhiko  
ONODERA Takuya  
Project Period (FY) 2012-04-01 – 2016-03-31
Keywordsブラックホール / X線観測 / X線新星 / 突発天体 / 新天体 / 連星進化 / 全天X線監視装置 MAXI / 国際宇宙ステーション
Outline of Final Research Achievements

The MAXI (Monitor of All-sky X-ray Image) nova-alert system to discover transient objects, such as X-ray novae, has been improved. As a result, the system can trigger on low flux variations near detection limits of GSC (Gas Slit Camera) detectors in realtime, and 11 X-ray transients including three black hole candidates were newly discovered. We have also established the method of the power spectrum analysis to investigate short-term variations during scan observations, and confirmed the state transition of black hole candidates from the power spectrum analysis. In addition, we developed a nova-alert system for SSC (Solid-state Slit Camera) data.

Free Research Field

X線天文学

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Published: 2017-05-10  

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