UV spectropolarimetry with Polstar: protoplanetary disks

Autor:	John P. Wisniewski, Andrei V. Berdyugin, Svetlana V. Berdyugina, William C. Danchi, Ruobing Dong, René D. Oudmaijer, Vladimir S. Airapetian, Sean D. Brittain, Ken Gayley, Richard Ignace, Maud Langlois, Kellen D. Lawson, Jamie R. Lomax, Evan A. Rich, Motohide Tamura, Jorick S. Vink, Paul A. Scowen
Rok vydání:	2022
Předmět:	Earth and Planetary Astrophysics (astro-ph.EP) Astrophysics::Instrumentation and Methods for Astrophysics FOS: Physical sciences Astronomy and Astrophysics Astrophysics::Cosmology and Extragalactic Astrophysics Astrophysics - Solar and Stellar Astrophysics Space and Planetary Science Astrophysics::Solar and Stellar Astrophysics Astrophysics::Earth and Planetary Astrophysics Astrophysics - Instrumentation and Methods for Astrophysics Instrumentation and Methods for Astrophysics (astro-ph.IM) Solar and Stellar Astrophysics (astro-ph.SR) Astrophysics::Galaxy Astrophysics Astrophysics - Earth and Planetary Astrophysics
Zdroj:	Astrophysics and Space Science. 367
ISSN:	1572-946X 0004-640X
Popis:	Polstar is a proposed NASA MIDEX mission that would feature a high resolution UV spectropolarimeter capable of measure all four Stokes parameters onboard a 60cm telescope. The mission would pioneer the field of time-domain UV spectropolarimetry. Time domain UV spectropolarimetry offers the best resource to determine the geometry and physical conditions of protoplanetary disks from the stellar surface to 16 pages, 7 figures
Databáze:	OpenAIRE
Externí odkaz:	https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e3e1ea43148b0575d49f23668b6195d4 https://doi.org/10.1007/s10509-022-04125-7 Zobrazit plný text záznamu Full text from SpringerLink