The transiting dust clumps in the evolved disc of the Sun-like UXor RZ Psc

RZ Psc is a young Sun-like star, long associated with the UXor class of variable stars, which is partially or wholly dimmed by dust clumps several times each year. The system has a bright and variable infrared excess, which has been interpreted as evidence that the dimming events are the passage of...

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Detalles Bibliográficos
Autores principales: Kennedy, Grant M., Kenworthy, Matthew A., Pepper, Joshua, Rodriguez, Joseph E., Siverd, Robert J., Stassun, Keivan G., Wyatt, Mark C.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: The Royal Society Publishing 2017
Materias:
Astronomy
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5319332/
https://www.ncbi.nlm.nih.gov/pubmed/28280566
http://dx.doi.org/10.1098/rsos.160652

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5319332/
https://www.ncbi.nlm.nih.gov/pubmed/28280566
http://dx.doi.org/10.1098/rsos.160652

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