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Black Hole Mass Scaling Relations of 10 Pseudo-Bulge Galaxies : 10개 수도벌지 은하의 블랙홀 질량 상관관계

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Authors

조국섭

Advisor
우종학
Major
자연과학대학 물리·천문학부(천문학전공)
Issue Date
2016-08
Publisher
서울대학교 대학원
Keywords
coevolutionpseudo-bulgesthe m-sigma relationgas kinematicsinclination effect
Description
학위논문 (석사)-- 서울대학교 대학원 : 물리·천문학부 천문학전공, 2016. 8. 우종학.
Abstract
We present stellar and gas kinematics of 10 pseudo-bulge galaxies, in order to investigate
the correlation between black hole mass (MBH) and galaxy properties, i.e., the
MBH-σ∗ relation (where σ∗ is stellar velocity dispersion) using high quality spatially
resolved spectra. We observed 9 galaxies with the Faint Object Camera and Spectrograph
(FOCAS) at the Subaru telescope, and the other with the Inamori Magellan
Areal Camera and Spectrograph (IMACS) at the Magellan telescope. For all galaxies,
we obtained spatially resolved data along the major axis and we measured the radial velocity
and velocity dispersion from stellar continuum and gas emission lines. We do not
find a significant evidence that pseudo-bulge galaxies offset from the MBH-σ∗ relation
based on the spatially resolved measurements. To investigate the inclination effects on
the effective sigma (σe), which defines the MBH-σ∗ relation, we calculated inclinationcorrected
σ∗. We suggest to use rotation-free σ∗ especially for galaxies with a rotation
dominant bulge, i.e., pseudo-bulges. Additionally, we obtained velocity and velocity
dispersion profiles of [OIII] and Hβ emission lines to investigate specific properties of
pseudo-bulge galaxies. Gas kinematics are generally following stellar kinematics, which
can be well explained by the gravitational potential of the host galaxies.
Language
English
URI
https://hdl.handle.net/10371/131673
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