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Orphaned Exomoons: Tidal Detachment and Evaporation Following an Exoplanet-Star Collision
Miguel Martinez, Nicholas C. Stone, Brian D. Metzger, 2019.
What it's used for here
MNRAS 489, 5119. An evaporating exomoon tidally detached after its planet's collision with the star feeds a dust disk; proposed to produce both the dips and the longer-term dimming.
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Research copy, for editors and curators. The work is the publisher's, so readers are sent to it. We keep this copy so the citation can be checked if the page changes or goes.
arxiv.org · fetched 30 Oct 2026
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Cite it
Miguel Martinez, Nicholas C. Stone, & Brian D. Metzger (2019). Orphaned Exomoons: Tidal Detachment and Evaporation Following an Exoplanet-Star Collision. https://doi.org/10.1093/mnras/stz2464
@article{martinez2019orphaned,
author = {Miguel Martinez} and {Nicholas C. Stone} and {Brian D. Metzger},
title = {Orphaned Exomoons: Tidal Detachment and Evaporation Following an Exoplanet-Star Collision},
year = {2019},
doi = {10.1093/mnras/stz2464},
url = {https://arxiv.org/abs/1906.08788}
}TY - JOUR TI - Orphaned Exomoons: Tidal Detachment and Evaporation Following an Exoplanet-Star Collision AU - Miguel Martinez AU - Nicholas C. Stone AU - Brian D. Metzger PY - 2019 DO - 10.1093/mnras/stz2464 UR - https://arxiv.org/abs/1906.08788 ER -
et al.. “Orphaned Exomoons: Tidal Detachment and Evaporation Following an Exoplanet-Star Collision.” 2019. https://doi.org/10.1093/mnras/stz2464.