Breakthroughs in Cool Star Physics with the Line Emission Mapper X-ray Probe
dc.contributor.author | Drake, Jeremy J. | |
dc.contributor.author | Gomez, Julián Alvarado | |
dc.contributor.author | Argiroffi, Costanza | |
dc.contributor.author | Flaccomio, Ettore | |
dc.contributor.author | Garraffo, Cecilia | |
dc.contributor.author | Grosso, Nicolas | |
dc.contributor.author | Islam, Nazma | |
dc.contributor.author | Karovska, Margarita | |
dc.contributor.author | Kashyap, Vinay L. | |
dc.contributor.author | Monsch, Kristina | |
dc.contributor.author | Ness, Jan-Uwe | |
dc.contributor.author | Sciortino, Salvatore | |
dc.contributor.author | Wargelin, Bradford | |
dc.date.accessioned | 2023-11-28T20:46:31Z | |
dc.date.available | 2023-11-28T20:46:31Z | |
dc.date.issued | 2023-10-26 | |
dc.description.abstract | We outline some of the highlights of the scientific case for the advancement of stellar high energy physics using the Line Emission Mapper X-ray Probe ({\it LEM}). The key to advancements with LEM lie in its large effective area -- up to 100 times that of the {\it Chandra} MEG -- and 1~eV spectral resolution. The large effective area opens up for the first time the ability to study time-dependent phenomena on their natural timescales at high resolution, such as flares and coronal mass ejections, and also opens the sky to much fainter targets than available to {\it Chandra} or {\it XMM-Newton}. | |
dc.description.uri | https://arxiv.org/abs/2310.17563 | |
dc.format.extent | 29 pages | |
dc.genre | white papers | |
dc.genre | preprints | |
dc.identifier.uri | https://doi.org/10.48550/arXiv.2310.17563 | |
dc.identifier.uri | http://hdl.handle.net/11603/30909 | |
dc.language.iso | en_US | |
dc.relation.isAvailableAt | The University of Maryland, Baltimore County (UMBC) | |
dc.relation.ispartof | UMBC Center for Space Sciences and Technology | |
dc.relation.ispartof | UMBC Faculty Collection | |
dc.relation.ispartof | UMBC Physics Department | |
dc.rights | This item is likely protected under Title 17 of the U.S. Copyright Law. Unless on a Creative Commons license, for uses protected by Copyright Law, contact the copyright holder or the author. | |
dc.title | Breakthroughs in Cool Star Physics with the Line Emission Mapper X-ray Probe | |
dc.type | Text | |
dcterms.creator | https://orcid.org/0000-0002-2413-9301 |