This National Science Foundation Project Grant award of $444,772 provides funding from September 1, 2022 through August 31, 2025 to study the evolution of magnetic complexity in old sun-like stars under the Mathematical and Physical Sciences program (CFDA 47.049). Principal investigators Metcalfe and Van Saders from the University of Hawaii at Manoa will take polarized spectra of 12 stars using the Potsdam Echelle Polarimetric and Spectroscopic Instrument at the Large Binocular Telescope and the...
This Project Grant award of $118,673 from the National Science Foundation's (NSF) Mathematical and Physical Sciences program (CFDA 47.049) supports a collaborative research project focused on "Polarimetric Asteroseismology of Massive Hot Stars." A team of astronomers from the Monterey Institute for Research in Astronomy, Florida Gulf Coast University, SETI Institute, University of Maryland Baltimore County, and University of Wisconsin-Madison, along with international partners, will...
This $145,866 Project Grant awarded by the National Science Foundation's (NSF) Division of Astronomical Sciences will fund a collaborative research initiative on "Polarimetric Asteroseismology of Massive Hot Stars." The project aims to determine the interior structures of these stars by observing seismic waves and applying a new polarimetric technique. The research team, comprising astronomers from Florida Gulf Coast University, Monterey Institute for Research in Astronomy, SETI...
The National Science Foundation awarded a $300,000 project grant under the Mathematical and Physical Sciences program to investigate magnetism and rotation in ultracool dwarfs and the smallest stars. With a completion date of November 2024, this funding will support research examining these phenomena in astronomical bodies through the lens of the Mathematical and Physical Sciences program's goal of strengthening the nation's scientific enterprise by increasing knowledge and understanding of...
The National Science Foundation (NSF) awarded a $422,670 Project Grant to the Monterey Institute for Research in Astronomy (MIRA) to support a collaborative research effort on "Polarimetric Asteroseismology of Massive Hot Stars". This research project, funded under the NSF's Mathematical and Physical Sciences (CFDA 47.049) program, aims to determine the interior structures of massive hot stars by applying a new technique called polarimetric asteroseismology. The collaboration...
The National Science Foundation (NSF) Division of Astronomical Sciences awarded a $318,113 Project Grant to the Massachusetts Institute of Technology (MIT) to conduct a collaborative research program entitled "A Comprehensive Theoretical Study of Cosmological Magnetic Fields and Turbulence: From the Early to Late Time Universe." This 3-year grant, which began on September 1, 2023, will support theoretical and computational modeling to investigate the origin, evolution, and...
The National Science Foundation (NSF) Division of Astronomical Sciences awarded a $420,110 Project Grant to the University of Wisconsin - Madison to "Explore Magnetic Fields on the Largest Scales." The 3-year award, beginning September 1, 2023, will fund research to develop a new "Gradient Technique" to map magnetic field directions in galaxy cluster "megahalos" - massive magnetic fields spanning millions of light years. The research aims to (1) test theories of the...
This Project Grant award from the National Science Foundation's (NSF) Mathematical and Physical Sciences program, with a total funding amount of $441,642, supports research to deepen the understanding of the final stages of stellar evolution, specifically focusing on red giants and their mass-shedding processes. The key objectives of this 2-year research project, which runs from September 1, 2024 to August 31, 2026, are to: Employ very long baseline interferometry (VLBI) observations,...
This $407,331 federal Project Grant award from the National Science Foundation's (NSF) Mathematical and Physical Sciences program supports research on magnetospheric accretion around magnetized stars. The University of Nevada, Las Vegas (UNLV) will conduct first-principle numerical simulations to study how neutron stars produce X-ray pulsars and ultraluminous X-ray sources, as well as how young stars and planets evolve within their environments. The research will include four key simulation...
This National Science Foundation (NSF) Mathematical and Physical Sciences project grant of $248,151 will support high resolution optical interferometry studies of interacting binary star systems to better understand stellar evolution and the formation of neutron stars and black holes. Led by Dr. [PI name] at New Mexico Institute of Mining and Technology, the team will use the Center for High Angular Resolution Astronomy array to collect interferometric data on known symbiotic binary stars over a...