27 citations
- The University of TokyoJP8 papers
- Aoyama Gakuin UniversityJP2 papers
- Hebrew University of JerusalemIL2 papers
- Hiroshima University of EconomicsJP2 papers
- Osaka University of TourismJP2 papers
- Saitama UniversityJP2 papers
- Ames Research CenterUS1 paper
- Amsterdam University CollegeNL1 paper
- Astronomical Institute of the Slovak Academy of SciencesSK1 paper
- Atmospheric Observatory of Austral PatagoniaAR1 paper
- California Institute of TechnologyUS1 paper
- Center for Astrophysics Harvard & SmithsonianUS1 paper
12 papers
Measuring the asymmetric expansion of the Fe ejecta of Cassiopeia A with XRISM/Resolve
Aya Bamba, Manan Agarwal, Jacco Vink +24
The expansion structure of supernova remnants (SNRs) is important for understanding not only how heavy elements are distributed into space, but also how supernovae explode. The eje…
Red Giant Winds Driven by Alfvén Waves with Magnetic Diffusion
Takeru K. Suzuki, Keiichi Ohnaka, Yuki Yasuda
We investigate the driving mechanism of Alfvén wave-driven stellar winds from red giant stars, Arcturus ( Boo; K1.5 III) and Aldebaran ( Tau; K5 III), with nonideal MHD simul…
On the X-ray efficiency of the white dwarf pulsar candidate ZTF J190132.9+145808.7
Aya Bamba, Yukikatsu Terada, Kazumi Kashiyama +3
Strongly magnetized, rapidly rotating massive white dwarfs (WDs) emerge as potential outcomes of double degenerate mergers. These WDs can act as sources of non-thermal emission and…
On the influence of shock-cloud interactions on the nonthermal X-ray emission from the supernova remnant RCW 86
Aya Bamba, Hidetoshi Sano, Ryo Yamazaki +1
It is an open issue how the surrounding environment of supernova remnant shocks affect nonthermal X-rays from accelerated electrons, with or without interacting dense material. We…
Ariel: Enabling planetary science across light-years
Giovanna Tinetti, Paul Eccleston, Carole Haswell +313
Ariel, the Atmospheric Remote-sensing Infrared Exoplanet Large-survey, was adopted as the fourth medium-class mission in ESA's Cosmic Vision programme to be launched in 2029. Durin…
FRB 181112 as a Rapidly-Rotating Massive Neutron Star just after a Binary Neutron Star Merger?: Implications for Future Constraints on Neutron Star Equations of State
Shotaro Yamasaki, Tomonori Totani, Kenta Kiuchi
The light curve of the fast radio burst (FRB) 181112 is resolved into four successive pulses, and the time interval ( ms) between the first and third pulses coincides with…