We report the discovery of 11 X-ray flares from 7 M dwarfs previously unknown to exhibit flaring activity, by cross-matching eROSITA observations of bright, nearby M dwarfs with the Chandra telescope archive. To analyze the properties of these flares in a broader context, we compile the sample of all reported X-ray flares from the 15 M dwarfs identified as flaring in the literature. We use this combined sample to derive constraints on the X-ray flare frequency distributions of M0-M6 stars. The average flare occurrence rate we measure is ∼10^−1 ks^−1 (corresponding to ∼9 flares per day). The X-ray flares in this sample span energies from 10^29erg to 10^33erg and exhibit a strong correlation between flare strength and duration. The flare properties we characterize include their durations, flux and temperature enhancements, and temporal asymmetries. Using these results and recent simulations of flare-driven atmospheric escape, we derive an upper limit on the time required for habitable Earth-like planets orbiting these M dwarfs to completely lose their atmospheres: 0.5-30 Myr.
", "publication_date": "2026-06-14", "publisher": "Zenodo", "resource_type": { "id": "poster", "title": { "de": "Poster", "en": "Poster" } }, "rights": [ { "description": { "en": "The Creative Commons Attribution license allows re-distribution and re-use of a licensed work on the condition that the creator is appropriately credited." }, "icon": "cc-by-icon", "id": "cc-by-4.0", "props": { "scheme": "spdx", "url": "https://creativecommons.org/licenses/by/4.0/legalcode" }, "title": { "en": "Creative Commons Attribution 4.0 International" } } ], "title": "Mapping the Landscape of M Dwarf X-ray Flares: New Discoveries in Context" }, "parent": { "access": { "owned_by": { "user": "1682957" }, "settings": { "accept_conditions_text": null, "allow_guest_requests": false, "allow_user_requests": false, "secret_link_expiration": 0 } }, "communities": { "default": "9ba7fd7e-a60f-4b7a-b3da-a178c21c5fda", "entries": [ { "access": { "member_policy": "open", "members_visibility": "public", "record_submission_policy": "open", "review_policy": "closed", "visibility": "public" }, "children": { "allow": false }, "created": "2026-04-06T12:19:20.716447+00:00", "custom_fields": { "subjects": [ { "id": "euroscivoc:769" }, { "id": "euroscivoc:763" }, { "id": "euroscivoc:1807" }, { "id": "euroscivoc:757" } ] }, "deletion_status": { "is_deleted": false, "status": "P" }, "id": "9ba7fd7e-a60f-4b7a-b3da-a178c21c5fda", "links": {}, "metadata": { "curation_policy": "All proceeding submissions will be reviewed by the curator(s) to ensure they are from registered conference attendees (in person or virtual) and adhere to the conference code of conduct.
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