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RCW 36
[CII] Emission Properties of the Massive Star-Forming Region
29 Jan 2020 11Department of Physics, Faculty of Science, Hokkaido University, Kita 10 Nishi 8, Kita-Ku, Sapporo, Hokkaido 060-0810, Japan
407 a Abell Galaxy Cluster S 373 (AGC S 373) , 351–353 Achromat
The Radio Spectral Index of the Vela Supernova Remnant
241 — 12 January 2013 Editor: Bo Reipurth (
[email protected]
)
X-Rays and Stellar Populations
Annual Report Volume 21 Fiscal 2018
Flux Calibration of the AAO/UKST Supercosmos Hα Survey
Contrat Quinquennal 2016‐2020
Characterizing the Outcome of Massive Star Formation?,??
Dr. QUANG NGUYEN-LUONG Assitant Professor, the American University of Paris Founder of BOLTZ.AI Data Scientist at Orthoevidence Inc
Star Formation in Nearby Clouds (Sfincs): X-Ray and Infrared Source Catalogs and Membership
Evidence for a High-Mass Star Cluster Formation Triggered by Cloud
Publications 2018
Uva-DARE (Digital Academic Repository)
Strategic Plan for Astronomy in the Netherlands 2011-2020
The Vela Supernova Remnant and the Gum Nebula
Molecular and Atomic Clouds Toward the Wolf-Rayet Nebula NGC 2359
Top View
A Multiwavelength Look at Galactic Massive Star Forming Regions
The Spatial Structure of Young Stellar Clusters. II
November 2018 BRAS Newsletter
Annual Report Publications 2013
The Vela Supernova Remnant and Surrounds – a Photographic Tour
Modeling of the Radio Emission from the Vela Supernova Remnant