TY - CHAP
T1 - Meter- to Millimeter Emission from Cool Stellar Systems
T2 - Latest Results, Synergies Across the Spectrum, and Outlook for the Next Decade
AU - Forbrich, Jan
AU - Williams, Peter K. G.
AU - Drabek-Maunder, Emily
AU - Howard, Ward
AU - Jardine, Moira
AU - Matthews, Lynn
AU - Moschou, Sofia
AU - Mutel, Robert
AU - Quiroga-Nuñez, Luis
AU - Rodriguez, Joseph
AU - Villadsen, Jackie
AU - Zic, Andrew
AU - Osten, Rachel
AU - Berger, Edo
AU - Güdel, Manuel
N1 - Splinter session summary, to appear in the proceedings of the 20th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun (ed. S. J. Wolk)
PY - 2018/11/1
Y1 - 2018/11/1
N2 - 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, JVLA, LOFAR), advances in related fields (e.g., the Gaia astrometric revolution), and above all a renewed interest in the relevant stellar astrophysics, stellar radio astronomy is experiencing a renaissance. In this splinter session, participants took stock of the present state of stellar radio astronomy to chart a course for the field's future.
AB - 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, JVLA, LOFAR), advances in related fields (e.g., the Gaia astrometric revolution), and above all a renewed interest in the relevant stellar astrophysics, stellar radio astronomy is experiencing a renaissance. In this splinter session, participants took stock of the present state of stellar radio astronomy to chart a course for the field's future.
KW - astro-ph.SR
U2 - 10.5281/zenodo.1476617
DO - 10.5281/zenodo.1476617
M3 - Chapter
SP - 1
EP - 8
BT - Proceedings of the 20th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun (ed. S. J. Wolk)
ER -