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UV spectropolarimetry with Polstar: protoplanetary disks
Journal article   Open access   Peer reviewed

UV spectropolarimetry with Polstar: protoplanetary disks

John P. Wisniewski, Andrei V. Berdyugin, Svetlana V. Berdyugina, William C. Danchi, Ruobing Dong, Rene D. Oudmaijer, Vladimir S. Airapetian, Sean D. Brittain, Ken Gayley, Richard Ignace, …
Astrophysics and space science, Vol.367(12), p.122
12/01/2022
DOI: 10.1007/s10509-022-04125-7

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Abstract

Polstar is a proposed NASA MIDEX mission that carries a high resolution UV spectropolarimeter capable of measure all four Stokes parameters onboard a 60 cm telescope. The mission has been designed to 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 < 5 AU. We detail two key objectives that a dedicated time domain UV spectropolarimetry survey, such as that enabled by Polstar or a similar mission concept, could achieve: 1) Test the hypothesis that magneto-accretion operating in young planet-forming disks around lower-mass stars transitions to boundary layer accretion in planet-forming disks around higher mass stars; and 2) Discriminate whether transient events in the innermost regions of planet-forming disks of intermediate mass stars are caused by inner disk mis-alignments or from stellar or disk emissions.
Physical Sciences Astronomy & Astrophysics Science & Technology

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