• 한국동물학회:학술대회논문집
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• 한국동물학회 2006년도 제61회 한국생물과학협회 정기학술대회
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• pp.10-10
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• 2006

• The Korean Journal of Physiology
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• 제25권1호
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• 1991

• 대한예방의학회:학술대회논문집
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• pp.285-292
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• 1994

• 천문학회보
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• 제32권1호
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• 2007

• 한국응용곤충학회:학술대회논문집
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• 한국응용곤충학회 2002년도 추계 합동 특강 및 학술발표대회
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• 2002

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• 한국잠사학회 2002년도 Join Meetings of Korean Society of Sericultural Science and Japanse Society of Sericultural Science
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• pp.57-57
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• 2002

No Abstract, See Full Text

• 천문학회보
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• 제35권2호
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• pp.28.1-28.1
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• 2010

Recent surveys have shown that many early-type galaxies have signatures of ongoing or recent star formation (RSF). These RSF galaxies show blue integrated UV-optical colours that set them aside in the NUV integrated colour-magnitude relation. Among them, NGC 4150 has been observed using the Wide Field Camera 3 (WFC3) on board the Hubble Space Telescope to inspect the galaxy with higher spatial resolution. In the WFC3 data, the galaxy reveals ubiquitous near-UV emission and remarkable dusty substructure. Our analysis shows this galaxy to lie in the near-UV green valley, and its pixel-by-pixel photometry exhibits a narrow range of UV-optical colours that are similar to those of nearby E+A (post-starburst) galaxies, and lie between those of M83 (an actively star-forming spiral) and the local quiescent early-type galaxy population. This work reaffirms our hypothesis that minor mergers play a significant role in the evolution of early-type galaxies at late epochs.

• 한국우주과학회:학술대회논문집(한국우주과학회보)
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• 한국우주과학회 2002년도 한국우주과학회보 제11권2호
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• pp.57-57
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• 2002

• 천문학회보
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• 제33권2호
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• pp.45.2-45.2
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• 2008

• 천문학회보
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• 제30권1호
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• 2005