Search Publications

Near-ultraviolet radiation toward molecular cloud N4 in W 50/SS 433: Evidence for direct interaction of the jet with molecular cloud
DOI: 10.1093/pasj/psae007 Bibcode: 2024PASJ...76L...1Y

Takeuchi, Tsutomu T.; Yamamoto, Hiroaki; Ishikawa, Tatsumi

We compared the molecular clouds in the western part of SS 433 with near-ultraviolet radiation data obtained from GALEX. Near-ultraviolet radiation is prominently confirmed toward only N4, while no near-ultraviolet radiation is detected toward N1, N2, or N3. The radiative region of near-ultraviolet radiation is nearly the same as the CO-emitting r…

2024 Publications of the Astronomical Society of Japan
AKARI 0
Discovery of diffuse radio source in Abell 1060
DOI: 10.1093/pasj/psae011 Bibcode: 2024PASJ...76L...8K

Nakazawa, Kazuhiro; Akahori, Takuya; Kurahara, Kohei +2 more

Non-thermal components in the intra-cluster medium (ICM), such as turbulence, magnetic field, and cosmic rays, imprint the past and current energetic activities of jets from active galactic nuclei (AGN) of member galaxies as well as disturbance caused by galaxy cluster mergers. Meter- and centimeter-radio observations of synchrotron radiation allo…

2024 Publications of the Astronomical Society of Japan
XMM-Newton 0
MK-like spectral classification for hot subdwarf stars with LAMOST spectra
DOI: 10.1093/pasj/psae072 Bibcode: 2024PASJ...76.1084Z

Lei, Zhenxin; Zou, Xuan

An MK-like spectral classification has been conducted for 1224 hot subdwarf stars with LAMOST DR9 low-resolution spectra. The whole sample was divided into four categories according to the spectral line characteristics: He-normal, He-weak, He-strong C, and He-strong. Each selected spectrum was assigned a spectral class, a luminosity class, and a h…

2024 Publications of the Astronomical Society of Japan
Gaia 0
Plasma diagnostics of supernova remnant 3C 400.2 by Suzaku observations
DOI: 10.1093/pasj/psae081 Bibcode: 2024PASJ...76.1202O

Nobukawa, Masayoshi; Uchiyama, Hideki; Nobukawa, Kumiko K. +2 more

We report on the results of plasma diagnostics of the supernova remnant (SNR) 3C 400.2, which has been reported to have a recombining plasma by previous studies. For careful background estimation, we simultaneously fitted spectra extracted from the SNR and background regions and evaluated the SNR emission contaminating the background-region spectr…

2024 Publications of the Astronomical Society of Japan
Suzaku 0
Low abundances of TiO and VO on the dayside of KELT-9 b: Insights from ground-based photometric observations
DOI: 10.1093/pasj/psae075 Bibcode: 2024PASJ...76.1131H

Ikuta, Kai; Fukui, Akihiko; Narita, Norio +21 more

We present ground-based photometric observations of secondary eclipses of the hottest known planet KELT-9 b using MuSCAT2 and Sinistro. We detect secondary eclipse signals in i and $z_{\rm s}$ with eclipse depths of

2024 Publications of the Astronomical Society of Japan
CHEOPS eHST 0
Dark matter search in the Perseus cluster with simultaneous analysis of Hitomi and Suzaku data
DOI: 10.1093/pasj/psae027 Bibcode: 2024PASJ...76..512F

Kitamoto, Shunji; Sawada, Makoto; Tamura, Takayuki +1 more

The reported detection of a 3.5 keV emission line in the Perseus cluster, possibly originating from dark matter decay, is still under scrutiny. Despite extensive observations, the detection has not yet been confirmed, and its origin remains a topic of active debate. Most of the previous searches relied on spectroscopy with X-ray charge-coupled dev…

2024 Publications of the Astronomical Society of Japan
Hitomi Suzaku 0