Search Publications

CO multi-line imaging of nearby galaxies (COMING). XII. CO-to-H2 conversion factor and dust-to-gas ratio
DOI: 10.1093/pasj/psad034 Bibcode: 2023PASJ...75..743Y

Kobayashi, Masato I. N.; Kuno, Nario; Miyamoto, Yusuke +8 more

We simultaneously measured the spatially resolved CO-to-H2 conversion factor (αCO) and dust-to-gas ratio (DGR) in nearby galaxies on a kiloparsec scale. In this study, we used 12CO(J = 1-0) data obtained by the Nobeyama 45 m radio telescope with H I and dust mass surface densities. We obtained the values of global …

2023 Publications of the Astronomical Society of Japan
Herschel 8
Cosmic-ray-driven enhancement of the C0/CO abundance ratio in W 51 C
DOI: 10.1093/pasj/psad046 Bibcode: 2023PASJ...75..883Y

Yamagishi, Mitsuyoshi; Kaneda, Hidehiro; Shimonishi, Takashi +5 more

We examine spatial variations of the C0$/$CO abundance ratio (XC/CO) in the vicinity of the γ-ray supernova remnant W 51 C, based on [C I] (3P1-3P0), 12CO(1-0), and 13CO(1-0) observations with the ASTE and Nobeyama 45 m telescopes. We find that XC/CO

2023 Publications of the Astronomical Society of Japan
Herschel 2
Twisted magnetic field in star formation processes of L1521 F revealed by submillimeter dual-band polarimetry using the James Clerk Maxwell Telescope
DOI: 10.1093/pasj/psac094 Bibcode: 2023PASJ...75..120F

Shinnaga, Hiroko; Tomisaka, Kohji; Harada, Naoto +3 more

Understanding the initial conditions of star formation requires both observational studies and theoretical works taking into account the magnetic field, which plays an important role in star formation processes. Herein, we study the young nearby dense cloud core L1521 F [n(H2) ~104-6 cm-3] in the Taurus Molecular C…

2023 Publications of the Astronomical Society of Japan
Herschel 2