C.-H. R. Chen
Max Planck Society
5 Papers
1 Citations
C.-H. R. Chen is an academic researcher from Max Planck Society. The author has contributed to research in topics: Young stellar object & Galaxy. The author has an hindex of 4, co-authored 5 publications.
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Papers
Surveying the agents of galaxy evolution in the tidally stripped, low metallicity small Magellanic Cloud (SAGE-SMC). III. Young stellar objects
Marta Sewilo,Marta Sewilo,L. R. Carlson,J. Seale,Remy Indebetouw,Margaret Meixner,Barbara A. Whitney,Barbara A. Whitney,Thomas P. Robitaille,Joana M. Oliveira,Karl D. Gordon,Karl D. Gordon,Marilyn R. Meade,Brian Babler,Joseph L. Hora,Miwa Block,Karl Misselt,J. Th. van Loon,C.-H. R. Chen,Ed Churchwell,Bernie Shiao +20 more
TL;DR: In this article, the SAGE-SMC IRAC (3.6-8.0μm) and MIPS (24 and 70 μm) catalogs and images combined with near-infrared (JHK s ) and optical (UBVI) data were used to identify a population of intermediate-to high-mass young stellar objects (YSOs) in the SMC.
Star formation rates from young-star counts and the structure of the ISM across the NGC 346/N66 complex in the SMC
Sacha Hony,Dimitrios A. Gouliermis,Dimitrios A. Gouliermis,Frédéric Galliano,Maud Galametz,Diane Cormier,C.-H. R. Chen,Sami Dib,Sami Dib,Annie Hughes,Annie Hughes,Annie Hughes,Ralf S. Klessen,Ralf S. Klessen,Ralf S. Klessen,Julia Roman-Duval,Linda J. Smith,J.-P. Bernard,J.-P. Bernard,C. Bot,L. Carlson,Karl D. Gordon,Karl D. Gordon,Remy Indebetouw,Vianney Lebouteiller,Min-Young Lee,S. C. Madden,Margaret Meixner,Margaret Meixner,Joana M. Oliveira,Monica Rubio,Marc Sauvage,Ronin Wu +32 more
TL;DR: In this article, a power law fit to the data yields a steep relation with an exponent of 26±02, with simple assumptions for the gas-to-dust mass ratio and the duration of star formation.
63
•Journal Article
The HERschel Inventory of the Agents of Galaxy Evolution in the Magellanic Clouds, a HERschel Open Time Key Program
Margaret Meixner,P. Panuzzo,Julia Roman-Duval,Chad Engelbracht,Brian Babler,J. Seale,Sacha Hony,E. Montiel,Marc Sauvage,Karl D. Gordon,Karl Misselt,K. Okumura,P. Chanial,Tracy L. Beck,J.-P. Bernard,Alberto D. Bolatto,C. Bot,Martha L. Boyer,L. R. Carlson,Geoffrey C. Clayton,C.-H. R. Chen,Diane Cormier,Yasuo Fukui,Maud Galametz,Frédéric Galliano +24 more
TL;DR: The HERSChel Inventory of The Agents of Galaxy Evolution (HERITAGE) in the Magellanic Clouds project is a Herschel Space Observatory open-time key program as mentioned in this paper, which is used to study the life cycle of matter as traced by dust in the LMC and SMC.
Herschel spectroscopy of massive young stellar objects in the Magellanic Clouds
Joana M. Oliveira,J. Th. van Loon,M. Sewilo,M. Sewilo,Min-Young Lee,Min-Young Lee,Vianney Lebouteiller,C.-H. R. Chen,D. Cormier,Miroslav Filipovic,L. R. Carlson,Remy Indebetouw,Remy Indebetouw,S. C. Madden,Margaret Meixner,Margaret Meixner,Benjamin A. Sargent,Yasuo Fukui +17 more
TL;DR: In this article, the spectral properties of massive Young Stellar Objects (YSOs) in the Large and Small Magellanic Clouds (LMC and SMC) were analyzed using the Herschel Space Observatory Photodetector Array Camera and Spectrometer (PACS).
The Herschel revolution: unveiling the morphology of the high mass star formation sites N44 and N63 in the LMC
Sacha Hony,Frédéric Galliano,S. C. Madden,P. Panuzzo,Margaret Meixner,Chad Engelbracht,Karl Misselt,Maud Galametz,Marc Sauvage,Julia Roman-Duval,Karl D. Gordon,Brandon Lawton,J.-P. Bernard,Alberto D. Bolatto,K. Okumura,C.-H. R. Chen,Remy Indebetouw,Frank P. Israel,E. Kwon,Aigen Li,Francisca Kemper,M. S. Oey,Monica Rubio +22 more
TL;DR: In this paper, the authors studied the structure of the medium surrounding sites of high-mass star formation to determine the interrelation between the HII regions and the environment from which they were formed.