16 citations
- California Institute of TechnologyUS7 papers
- Moscow Institute of Thermal TechnologyRU7 papers
- National Institute for AstrophysicsIT7 papers
- Stanford UniversityUS6 papers
- Princeton UniversityUS5 papers
- University of MichiganUS5 papers
- University of WashingtonUS5 papers
- Center for Astrophysics Harvard & SmithsonianUS4 papers
- CFA InstituteUS4 papers
- Columbia UniversityUS4 papers
- University of California, BerkeleyUS4 papers
- University of Wisconsin–MadisonUS4 papers
18 papers · 1 filter
Activity Cycles of Southern Asteroseismic Targets
T. S. Metcalfe, P. G. Judge, S. Basu +4
The Mount Wilson Ca HK survey revealed magnetic activity variations in a large sample of solar-type stars with timescales ranging from 2.5 to 25 years. This broad range of cycle pe…
Structure and Evolution of Pre-Main Sequence Stars
Norbert S. Schulz, Glenn Allen, Mark W. Bautz +28
Low-mass pre-main sequence (PMS) stars are strong and variable X-ray emitters, as has been well established by EINSTEIN and ROSAT observatories. It was originally believed that thi…
From Protostars to Planetary Systems : FUV Spectroscopy of YSOs, Protoplanetary Disks, and Extrasolar Giant Planets
Paul A. Scowen, Rolf Jansen, Matthew Beasley +7
The last two decades have seen remarkable progress in our long-standing goal of determining the abundance and diversity of worlds in the Galaxy. Understanding of this subject invol…
The Star Formation Camera
Paul A. Scowen, Rolf Jansen, Matthew Beasley +21
The Star Formation Camera (SFC) is a wide-field (~15'x19, >280 arcmin^2), high-resolution (18x18 mas pixels) UV/optical dichroic camera designed for the Theia 4-m space-borne space…
The Magellanic Clouds Survey: a Bridge to Nearby Galaxies
Paul A. Scowen, Rolf Jansen, Matthew Beasley +7
We outline to the community the value of a Magellanic Clouds Survey that consists of three components: I) a complete-area, high resolution, multi-band UV-near-IR broadband survey;…
X-ray Cluster Cosmology
A. Vikhlinin, S. Murray, R. Gilli +18
Sensitive, wide-area X-ray surveys which would be possible with the WFXT will detect huge samples of virialized objects spanning the mass range from sub-groups to the most massive…