papers

Publications (81)

astro-ph.SR2014

CSI 2264: Simultaneous optical and infrared light curves of young disk-bearing stars in NGC 2264 with CoRoT and Spitzer-- evidence for multiple origins of variability

Ann Marie Cody, John Stauffer, Annie Baglin +42

We present the Coordinated Synoptic Investigation of NGC 2264, a continuous 30-day multi-wavelength photometric monitoring campaign on more than 1000 young cluster members using 16…

astro-ph.GA2018

The ALMA view of GMCs in NGC 300: Physical Properties and Scaling Relations at 10 pc Resolution

Christopher M. Faesi, Charles J. Lada, Jan Forbrich

We have conducted a CO(2-1) survey of several molecular gas complexes in the vicinity of H II regions within the spiral galaxy NGC 300 using the Atacama Large Millimeter Arr…

astro-ph.SR2018

Meter- to Millimeter Emission from Cool Stellar Systems: Latest Results, Synergies Across the Spectrum, and Outlook for the Next Decade

Jan Forbrich, Peter K. G. Williams, Emily Drabek-Maunder +12

Radio observations of cool stellar systems provide unique information on their magnetic fields, high-energy processes, and chemistry. Buoyed by powerful new instruments (e.g. ALMA,…

astro-ph.GA2026

Resolved Dust Emission and CO Isotopologues in Giant Molecular Clouds of the Andromeda Galaxy

Chloe Bosomworth, Jan Forbrich, Charles J. Lada +1

Dust emission at submillimeter wavelengths can be used to reliably trace the basic properties of molecular clouds. Early results from a recent Submillimeter Array (SMA) survey of t…

astro-ph.SR2020

A VLBA Survey of radio stars in the Orion Nebula Cluster: II. Astrometry

Sergio A. Dzib, Jan Forbrich, Mark J. Reid +1

From Very Long Baseline Array (VLBA) observations we previously identified a population of 123 young stellar systems with nonthermal radio emission toward the core of the Orion Neb…

astro-ph.GA2025

The SKA Galactic Centre Survey -- A White Paper

Rainer Schoedel, Antxon Alberdi, Izaskun Jimenez-Serra +17

With its extreme density of stars and stellar remnants, dense young massive clusters, high specific star formation rate, intense radiation field, high magnetic field strength, and…