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- Institute of Astronomy and Astrophysics, Academia SinicaTW117 papers
- National Taiwan UniversityTW111 papers
- Centre National de la Recherche ScientifiqueFR98 papers
- National Astronomical Observatory of JapanJP91 papers
- Chinese Academy of SciencesCN90 papers
- The University of TokyoJP88 papers
- California Institute of TechnologyUS86 papers
- Institute of Physics, Academia SinicaTW84 papers
- National Tsing Hua UniversityTW79 papers
- Korea Astronomy and Space Science InstituteKR77 papers
- The Graduate University for Advanced Studies, SOKENDAIJP77 papers
- Peking UniversityCN75 papers
47 papers · 1 filter
A Dual-Band Centimetre Continuum Monitoring Survey of Young Stellar Objects in the Coronet Cluster
Johanan Ramírez-Arellano, Carlos Carrasco-González, Roberto Galván-Madrid +5
We present sensitive (9 Jy), sub-arcsecond resolution radio continuum observations at 9.0 GHz (3.3 cm) and 14.0 GHz (2.1 cm) obtained with the Karl G. Jansky Very Large Ar…
Full-polarization millimeter wavelength variability of Sagittarius A* during the 2018 EHT campaign
Ezequiel Albentosa-Ruiz, Jasmin E. Washington, Nicola Marchili +272
Sagittarius A* (Srg A*), the supermassive black hole at the center of the Milky Way, provides a unique laboratory to study accretion dynamics and plasma processes near the event ho…
Linear filament and nested cluster evolution tomography (LANCET) I. Capture the evolution of dense gas in 14-parsec filament G316.8
Fengwei Xu, Ke Wang, Nicola Schneider +12
A dynamic view of mass assembly is essential for understanding the formation of massive stars and clusters. Interpreting evolutionary diagnostics from Galactic-wide surveys, howeve…
The Rotation Dip in the Envelope-Disk Transition of HH 111: Evidence for Magnetic Braking
Jyun-Heng Lin, Chin-Fei Lee, Zhi-Yun Li +3
Magnetic braking can drive angular momentum loss in star formation and influence disk evolution. A previous study of HH 111 VLA1 suggested a decrease in rotation velocity in a regi…
The Nearby Evolved Stars Survey III: First data release of JCMT CO-line observations
S. H. J. Wallström, P. Scicluna, S. Srinivasan +37
Low- to intermediate-mass (0.88 M) evolved stars contribute significantly to the chemical enrichment of the interstellar medium in the local Universe, making accur…
An S-shaped filament formed due to Cloud-Cloud Collision in molecular cloud G178.28-00.61
Tianwei Zhang, Tie Liu, Yuefang Wu +18
We present compelling observational evidence supporting G178.28-00.61 as an early-stage candidate for Cloud-Cloud Collision (CCC), with indications of the formation of an S-shaped…