Survey of active solar-type stars with the wide-filed photometric observations and archival data
Project/Area Number |
26800096
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Research Category |
Grant-in-Aid for Young Scientists (B)
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Allocation Type | Multi-year Fund |
Research Field |
Astronomy
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Research Institution | National Astronomical Observatory of Japan |
Principal Investigator |
Maehara Hiroyuki 国立天文台, 岡山天体物理観測所, 専門研究職員 (40456851)
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Research Collaborator |
Shibata Kazunari 京都大学, 大学院理学研究科, 教授 (70144178)
Nogami Daisaku 京都大学, 大学院理学研究科, 准教授 (20332728)
Honda Satoshi 兵庫県立大学, 天文科学センター, 特任助教 (20425408)
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Project Period (FY) |
2014-04-01 – 2017-03-31
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Project Status |
Completed (Fiscal Year 2016)
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Budget Amount *help |
¥3,770,000 (Direct Cost: ¥2,900,000、Indirect Cost: ¥870,000)
Fiscal Year 2016: ¥780,000 (Direct Cost: ¥600,000、Indirect Cost: ¥180,000)
Fiscal Year 2015: ¥650,000 (Direct Cost: ¥500,000、Indirect Cost: ¥150,000)
Fiscal Year 2014: ¥2,340,000 (Direct Cost: ¥1,800,000、Indirect Cost: ¥540,000)
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Keywords | 恒星フレア / 光赤外線天文学 / 恒星物理学 / 恒星黒点 / 太陽型星 / 黒点 / スーパーフレア / フレア |
Outline of Final Research Achievements |
Previous studies by using the data from Kepler suggest that a part of solar-type stars with the rotation period comparable to the Sun (~25 days) show much higher magnetic activity (e.g., superflares). We studied the rotation period distribution of the solar-type stars with high X-ray luminosity from grand-based photometric and spectroscopic observations. We found that some of active solar-type stars have the rotation velocity of < 5 km/s. We also studied the statistical properties of superflares on active solar-type stars by using the Kepler 1-min cadence data. We found a clear correlation between the duration of flares and the energy released by flares. This correlation can be explained if we assume that flares are caused by the magnetic reconnection.
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Report
(4 results)
Research Products
(20 results)
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[Journal Article] Starspot activity and superflares on solar-type stars2017
Author(s)
Maehara, H., Notsu, Y., Notsu, S., Namekata, K., Honda, S., Ishii, T., T., Nogami, D., and Shibata, K.
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Journal Title
Publications of the Astronomical Society of Japan
Volume: 印刷中
Issue: 3
Pages: 41-41
DOI
Related Report
Peer Reviewed / Acknowledgement Compliant
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[Journal Article] Spectroscopic observations of active solar-analog stars with high X-ray luminosity, as a proxy of superflare stars2017
Author(s)
Notsu, Y., Honda, S., Maehara, H., Notsu, S., Namekata, K., Nogami, D., and Shibata, K.
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Journal Title
Publications of the Astronomical Society of Japan
Volume: 69
Issue: 1
Pages: 12-12
DOI
Related Report
Peer Reviewed / Acknowledgement Compliant
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[Journal Article] High-dispersion spectroscopy of solar-type superflare stars. I. Temperature, surface gravity, metallicity, and vsin i2015
Author(s)
Notsu, Y., Honda, S.,Maehara, H., Notsu, S., Shibayama, T., Nogami, D., Shibata, K.
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Journal Title
Publications of the Astronomical Society of Japan
Volume: -
Issue: 3
Pages: 32-32
DOI
Related Report
Peer Reviewed / Open Access / Acknowledgement Compliant
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[Journal Article] Two sun-like superflare stars rotating as slow as the Sun*2014
Author(s)
Nogami, D., Notsu, Y., Honda, S., Maehara, H., Notsu, S., Shibayama, T., Shibata, K.
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Journal Title
Publications of the Astronomical Society of Japa
Volume: 66
Issue: 2
DOI
NAID
Related Report
Peer Reviewed / Open Access
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[Journal Article] Superflare Occurrence and Energies on G-, K-, and M-type Dwarfs2014
Author(s)
Candelaresi, S., Hillier, A., Maehara, H., Brandenburg, A., Shibata, K.
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Journal Title
The Astrophysical Journal
Volume: 792
Issue: 1
Pages: 67-67
DOI
Related Report
Peer Reviewed / Open Access
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