Exploring galaxies and supermassive black holes in the earliest phase of their chemical evolution
Project/Area Number |
23654068
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Research Category |
Grant-in-Aid for Challenging Exploratory Research
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Allocation Type | Multi-year Fund |
Research Field |
Astronomy
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Research Institution | Ehime University (2013) Kyoto University (2011-2012) |
Principal Investigator |
NAGAO Tohru 愛媛大学, 宇宙進化研究センター, 教授 (00508450)
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Co-Investigator(Kenkyū-buntansha) |
KAWAKATSU Nozomu 呉工業高等専門学校, 自然科学系分野, 准教授 (30450183)
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Project Period (FY) |
2011 – 2013
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Project Status |
Completed (Fiscal Year 2013)
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Budget Amount *help |
¥3,380,000 (Direct Cost: ¥2,600,000、Indirect Cost: ¥780,000)
Fiscal Year 2013: ¥780,000 (Direct Cost: ¥600,000、Indirect Cost: ¥180,000)
Fiscal Year 2012: ¥910,000 (Direct Cost: ¥700,000、Indirect Cost: ¥210,000)
Fiscal Year 2011: ¥1,690,000 (Direct Cost: ¥1,300,000、Indirect Cost: ¥390,000)
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Keywords | 銀河進化 / 光学赤外線天文学 / 巨大ブラックホール / 化学進化 / 電離ガス / スペクトル解析 / 電波天文学 / 銀河天文学 / 活動銀河核 / 宇宙化学進化 / 光電離モデル / 宇宙物理 |
Research Abstract |
For exploring extremely metal-poor galaxies at the initial phase of their chemical evolution in nearby (i.e., current) universe, we performed wide-field narrow-band imaging observations and follow-up deep spectroscopic observations. Accordingly we found 20 galaxies emitting [OIII]4363 emission, that is expected for such metal-poor galaxies. On the other hand, we investigated also the chemical properties of galaxies hosting supermassive black holes in nearby (i.e., current) universe, through the analysis of UV spectra of PG quasars. As a result, the inferred statistical dependences of their chemical properties on the mass accretion rate onto their supermassive black holes are systematically different between the nearby and distant universe. This infers a systematically different physics behind the mass fueling onto supermassive black holes at the nucleus of galaxies.
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Report
(4 results)
Research Products
(78 results)
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[Journal Article] ALMA resolves turbulent, rotating [CII] emission in a young starburst galaxy at z=4.82014
Author(s)
C. De Breuck, R. Williams, M. Swinbank, P. Caselli, K. Coppin, T. Davis, R. Maiolino, T. Nagao, I. Smail, F. Walter, A. Weiss, and M. Zwaan
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Journal Title
Astronomy and Astrophysics
Volume: Volume565
Pages: A59-A59
DOI
Related Report
Peer Reviewed
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[Journal Article] Metallicity evolution, metallicity gradients, and gas fractions at z~3.42014
Author(s)
Troncoso, P.; Maiolino, R.; Sommariva, V.; Cresci, G.; Mannucci, F.; Marconi, A.; Meneghetti, M.; Grazian, A.; Cimatti, A.; Fontana, A.; Nagao, T.; Pentericci, L.
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Journal Title
Astronomy and Astrophysics
Volume: 563
Pages: A58-A58
DOI
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Peer Reviewed
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[Journal Article] Flaring up of the compact cloud G2 during the close encounter with Sgr A*2014
Author(s)
Saitoh, Takayuki R.; Makino, Junichiro; Asaki, Yoshiharu; Baba, Junichi; Komugi, Shinya; Miyoshi, Makoto; Nagao, Tohru; Takahashi, Masaaki; Takeda, Takaaki; Tsuboi, Masato; Wakamatsu, Ken-ichi
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Journal Title
Publications of the Astronomical Society of Japan
Volume: 66
Issue: 1
Pages: 1-9
DOI
Related Report
Peer Reviewed
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[Journal Article] ALMA resolves turbulent, rotating [CII] emission in a young starburst galaxy at z=4.82014
Author(s)
De Breuck, C.; Williams, R.; Swinbank, M.; Caselli, P.; Coppin, K.; Davis, T.; Maiolino, R.; Nagao, T.; Smail, I.; Walter, F.; Weiss, A.; and Zwaan, M.
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Journal Title
Astronomy and Astrophysics
Volume: 未定
Related Report
Peer Reviewed
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[Journal Article] Strongly star-forming rotating disks in a complex merging system at z = 4.7 as revealed by ALMA2013
Author(s)
Carniani, S.; Marconi, A.; Biggs, A.; Cresci, G.; Cupani, G.; D'Odorico, V.; Humphreys, E.; Maiolino, R.; Mannucci, F.; Molaro, P.; Nagao, T.; Testi, L.; Zwaan, M. A.
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Journal Title
Astronomy and Astrophysics
Volume: 559
Pages: A29-A29
DOI
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Peer Reviewed
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[Journal Article] Resolved [CII] Emission in a Lensed Quasar at z=4.42012
Author(s)
Gallerani, Neri, Maiolino, Martin, De Breuck, Walter, Caselli, Krips, Meneghetti, Nagao, Wagg, and Walmsley
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Journal Title
Astronomy and Astrophysics
Volume: 543
Pages: A114-A114
DOI
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Peer Reviewed
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[Journal Article] ALMA reveals a chemically evolved submillimeter galaxy at z = 4.762012
Author(s)
Nagao, T., Maiolino, R., De Breuck, C., Caselli, P., Hatsukade, B., Saigo, K
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Journal Title
Astronomy and Astrophysics
Volume: Vol.542
Pages: L34-L34
DOI
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Peer Reviewed
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[Journal Article] Dynamical properties of AMAZE and LSD galaxies from gas kinematics and the Tully-Fisher relation at z~32011
Author(s)
A. Gnerucci, A. Marconi, G. Cresci, R. Maiolino, F. Mannucci, F. Calura, A. Cimatti, F. Cocchaia, A. Grazian, F. Matteucci, T. Nagao, L. Pozzetti, and P. Troncoso
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Journal Title
Astronomy and Astrophysics
Volume: Volume528
Pages: A88-A88
DOI
Related Report
Peer Reviewed
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[Journal Article] Spectropolarimetric Evidence for Radiatively Inefficient Accretion in an Optically Dull Active Galaxy2011
Author(s)
J. Trump, T. Nagao, H. Ikeda, T. Murayama, C. Impey, J. Stocke, F. Civano, M. Elvis, K. Jahnke, B. Kelly, A. Koekemoer, Y. Taniguchi
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Journal Title
The Astrophysical Journal
Volume: 732
Issue: 1
Pages: 23-23
DOI
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Peer Reviewed
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[Journal Article] Accretion Rate and the Physical Nature of Unobscured Active Galaxies2011
Author(s)
J. Trump, C. Impey, B. Kelly, F. Civano, J. Gabor, A. Diamond-Stanic, A. Merloni, M. Urry, H. Hao, K. Jahnke, T. Nagao, et al.
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Journal Title
The Astrophysical Journal
Volume: 733
Issue: 1
Pages: 60-60
DOI
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Peer Reviewed
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[Presentation] FIR-Submm metallicity diagnostics for high-z galaxies2012
Author(s)
T. Nagao, R. Maiolino, C. De Breuck, P. Caselli, A. Marconi, B. Hatsukade, K. Saigo, and H. Matsuhara
Organizer
国際研究会"European week of astronomy and space science : Symposium 1 : Molecular gas in high-z galaxies"
Place of Presentation
Pontifica Universita Lateranense, Rome (Italy)
Year and Date
2012-07-02
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