activity
20192026
most citedThe past, present and future of observations of externally irradiated disks

10 citations · 26 across the 9 of their papers we have counts for

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6 papers · 1 filter

astro-ph.GA2026

Low-Metallicity Star Formation Survey in Sh2-284 (LZ-STAR): The Core Mass Function

Yu Cheng, Jonathan C. Tan, Morten Andersen +4

We present an ALMA 1.3~mm dust continuum study of the dense core mass function (CMF) in Sh2-284, a low metallicity outer Galaxy star-forming complex with --.…

astro-ph.GA2025★ 3 cited

The JWST-NIRCam View of Sagittarius C. III. The Extinction Curve

Lucía Bravo Ferres, Francisco Nogueras-Lara, Rainer Schödel +8

Determining the infrared extinction curve towards the Galactic centre is crucial for accurately correcting observed data and deriving the underlying stellar populations. However, e…

astro-ph.GA2025

Low-Metallicity Star Formation Survey in Sh2-284 (LZ-STAR). I. Ordered massive star formation in the outer Galaxy

Yu Cheng, Jonathan C. Tan, Morten Andersen +5

Star formation is a fundamental, yet poorly understood, process of the Universe. It is important to study how star formation occurs in different galactic environments. Thus, here,…

astro-ph.GA2024★ 6 cited

The JWST-NIRCam View of Sagittarius C. II. Evidence for Magnetically Dominated HII Regions in the CMZ

John Bally, Samuel Crowe, Rubén Fedriani +11

We present JWST-NIRCam narrow-band, 4.05 m Brackett- images of the Sgr C HII region, located in the Central Molecular Zone (CMZ) of the Galaxy. Unlike any HII region in the S…

astro-ph.GA2024

The JWST-NIRCam View of Sagittarius C. I. Massive Star Formation and Protostellar Outflows

Samuel Crowe, Rubén Fedriani, Jonathan C. Tan +14

We present James Webb Space Telescope (JWST)-NIRCam observations of the massive star-forming molecular cloud Sagittarius C (Sgr C) in the Central Molecular Zone (CMZ). In conjuncti…

astro-ph.GA2019★ 1 cited

Star Formation in Different Environments: The Initial Mass Function

M. W. Hosek, J. R. Lu, M. Andersen +7

The stellar initial mass function (IMF) is a fundamental property of star formation, offering key insight into the physics driving the process as well as informing our understandin…