Correlation of MgII(h+k) UV Resonance Lines and Rotational Period in G-type Stars

Manuel Olmedo, Miguel Chávez, Emanuele Bertone

Research output: Chapter in Book/Report/Conference proceedingConference contribution

4 Citations (Scopus)
Original languageEnglish
Title of host publicationNew Quests in Stellar Astrophysics III: A Panchromatic View of Solar-Like Stars, With and Without Planets
EditorsM. Chavez, E. Bertone, O. Vega, V. De la Luz
PublisherPublications of the Astronomical Society of the Pacific
Pages267
Number of pages1
Volume472
DOIs
Publication statusPublished - 1 Apr 2013
Externally publishedYes

Publication series

NameAstronomical Society of the Pacific Conference Series

Cite this

Olmedo, M., Chávez, M., & Bertone, E. (2013). Correlation of MgII(h+k) UV Resonance Lines and Rotational Period in G-type Stars. In M. Chavez, E. Bertone, O. Vega, & V. De la Luz (Eds.), New Quests in Stellar Astrophysics III: A Panchromatic View of Solar-Like Stars, With and Without Planets (Vol. 472, pp. 267). (Astronomical Society of the Pacific Conference Series). Publications of the Astronomical Society of the Pacific. https://doi.org/10.1086/674332