39 citations
- Institute of Astronomy and Astrophysics, Academia SinicaTW3 papers
- National Taiwan UniversityTW2 papers
- California Institute of TechnologyUS1 paper
- Center for Astrophysics Harvard & SmithsonianUS1 paper
- Dalhousie UniversityCA1 paper
- Durham UniversityGB1 paper
- Fukuoka Institute of TechnologyJP1 paper
- Ghent UniversityBE1 paper
- Laboratoire d’études spatiales et d’instrumentation en astrophysiqueFR1 paper
- Laboratoire Interdisciplinaire Carnot de BourgogneFR1 paper
- Laboratoire Interuniversitaire des Systèmes AtmosphériquesFR1 paper
- Leiden UniversityNL1 paper
5 papers
CO-to-H conversion factor and grain size distribution through the analysis of - relation
I-Da Chiang, Hiroyuki Hirashita, Jeremy Chastenet +5
The CO-to-H conversion factor () is expected to vary with dust abundance and grain size distribution through the efficiency of shielding gas from CO-dissociation…
The Structure of Massive Star-Forming Galaxies from JWST and ALMA: Dusty, High Redshift Disk Galaxies
Steven Gillman, Ian Smail, Bitten Gullberg +15
We present an analysis of the JWST NIRCam and MIRI morphological properties of 80 massive (=11.20.1) dusty star-forming galaxies at 2.7$^{+…
Self and N2 collisional broadening of far-infrared methane lines at low-temperature with application to Titan
C. Richard, V. Boudon, L. Manceron +4
We report the measurement of broadening coefficients of pure rotational lines of methane at different pressure and temperature conditions. A total of 27 far-infrared spectra were r…
A Multiwavelength Survey of Wolf-Rayet Nebulae in the Large Magellanic Cloud
Clara Shang Hung, Po-Sheng Ou, You-Hua Chu +2
Surveys of Wolf-Rayet (WR) stars in the Large Magellanic Cloud (LMC) have yielded a fairly complete catalog of 154 known stars. We have conducted a comprehensive, multiwavelength s…
Intersection between pencils of tubes, discretized sum-product, and radial projections
Bochen Liu, Chun-Yen Shen
In this paper we prove the following results in the plane. They are related to each other, while each of them has its own interest. First we obtain an -increment on intersecti…