activity
20142026
most citedUV line driven disc wind as the origin of ultrafast outflows in AGN

50 citations · 703 across the 70 of their papers we have counts for

collaborators
Showing 2018Show all

7 papers · 1 filter

astro-ph.GA2018★ 27 cited

Kinetic energy transfer from X-ray ultrafast outflows to mm/sub-mm cold molecular outflows in Seyfert galaxies

Misaki Mizumoto, Takuma Izumi, Kotaro Kohno

UltraFast Outflows (UFOs), seen as X-ray blueshifted absorption lines in active galactic nuclei (AGNs), are considered to be a key mechanism for AGN feedback. In this scenario, UFO…

astro-ph.SR2018★ 2 cited

WINERED high-resolution near-infrared line catalog: A-type star

H. Sameshima, Y. Ikeda, N. Matsunaga +13

We present a catalog of absorption lines in the z', Y, and J bands that we identified in 21 Lyn, a slowly rotating A0.5 V star. We detected 155 absorption features in the high-reso…

astro-ph.SR2018★ 5 cited

A newly-identified emission-line region around P Cygni

Misaki Mizumoto, Naoto Kobayashi, Satoshi Hamano +12

We present a high-resolution () near-infrared (9,100-13,500 ) long-slit spectrum of P Cygni obtained with the newly commissioned WINERED spectrograph in Japan.…

astro-ph.HE2018★ 25 cited

X-ray reverberation lags of the Fe-K line due to AGN disc winds

Misaki Mizumoto, Ken Ebisawa, Masahiro Tsujimoto +3

Short X-ray reverberation lags are seen across a broad Fe-K energy band in more than twenty active galactic nuclei (AGNs). This broad iron line feature in the lag spectrum is most…

astro-ph.IM2018★ 31 cited

Correction of near-infrared high-resolution spectra for telluric absorption at 0.90-1.35 microns

Hiroaki Sameshima, Noriyuki Matsunaga, Naoto Kobayashi +15

We report a method of correcting a near-infrared (0.90-1.35 m) high-resolution () spectrum for telluric absorption using the corresponding spectrum of a telluric…

astro-ph.HE2018★ 26 cited

X-ray short-time lags in the Fe-K energy band produced by scattering clouds in active galactic nuclei

Misaki Mizumoto, Chris Done, Kouichi Hagino +3

X-rays illuminating the accretion disc in active galactic nuclei give rise to an iron K line and its associated reflection spectrum which are lagged behind the continuum variabilit…

astro-ph.HE2018★ 4 cited

Can the relativistic light bending model explain X-ray spectral variations of Seyfert galaxies?

Misaki Mizumoto, Kotaro Moriyama, Ken Ebisawa +3

Many Seyfert galaxies are known to exhibit Fe-K broad emission line features in their X-ray energy spectra. The observed lines have three distinct features; (1) the line profiles a…