output
20022026
most citedObservation of a resonance-like structure in the pi^+- psi' mass distribution in exclusive B-->K pi^+- psi' decays

550 citations

Showing astro-ph.SRShow all

25 papers · 1 filter

astro-ph.SR20262 cited

X-ray and Hα superflare on an RS CVn-type star, UX Arietis: Constraint on the flare location from radial velocity change during the flare

Sota Urabe, Yohko Tsuboi, Kosuke Namekata +5

We report on a giant stellar flare from the RS CVn-type binary UX Arietis, detected with the Monitor of All-sky X-ray Image (MAXI) and followed by a 12-day optical spectroscopic ca…

astro-ph.SR20251 cited

FAUST XXX: Dust enhancement in the young binary L1551 IRS 5

Nicolás Cuello, Eleonora Bianchi, François Ménard +17

Young binary stars with discs provide unique laboratories to study the earliest stages of planet formation in star-forming environments. The detection of substructure in discs arou…

astro-ph.SR20231 cited

Scale-dependent analysis of angular momentum flux in high-resolution magnetohydrodynamic simulations for solar differential rotation

K. Mori, H. Hotta

In this work, we systematically investigate the scale-dependent angular momentum flux by analysing high-resolution three-dimensional magnetohydrodynamic simulations in which the so…

astro-ph.SR20237 cited

Magnetohydrodynamic Model of Late Accretion onto a Protoplanetary Disk: Cloudlet Encounter Event

Masaki Unno, Tomoyuki Hanawa, Shinsuke Takasao

Recent observations suggest late accretion, which is generally nonaxisymmetric, onto protoplanetary disks. We investigated nonaxisymmetric late accretion considering the effects of…

astro-ph.SR20228 cited

Impact of subsurface convective flows on the formation of sunspot magnetic field and energy build-up

Takafumi Kaneko, Hideyuki Hotta, Shin Toriumi +1

Strong solar flares occur in -spots characterized by the opposite-polarity magnetic fluxes in a single penumbra. Sunspot formation via flux emergence from the convection zone to…

astro-ph.SR20226 cited

Mean-field analysis on large-scale magnetic fields at high Reynolds numbers

Ryota Shimada, Hideyuki Hotta, Takaaki Yokoyama

Solar magnetic fields comprise an 11-year activity cycle, represented by the number of sunspots. The maintenance of such a solar magnetic field can be attributed to fluid motion in…