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

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

Correlation of MgII(h+k) UV Resonance Lines and Rotational Period in G-type Stars. / Olmedo, Manuel; Chávez, Miguel; Bertone, Emanuele.

New Quests in Stellar Astrophysics III: A Panchromatic View of Solar-Like Stars, With and Without Planets. ed. / M. Chavez; E. Bertone; O. Vega; V. De la Luz. Vol. 472 Publications of the Astronomical Society of the Pacific, 2013. p. 267 (Astronomical Society of the Pacific Conference Series).

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

TY - GEN

T1 - Correlation of MgII(h+k) UV Resonance Lines and Rotational Period in G-type Stars

AU - Olmedo, Manuel

AU - Chávez, Miguel

AU - Bertone, Emanuele

PY - 2013/4/1

Y1 - 2013/4/1

UR - http://adsabs.harvard.edu/abs/2013PASP..125.1436O

U2 - 10.1086/674332

DO - 10.1086/674332

M3 - Conference contribution

VL - 472

T3 - Astronomical Society of the Pacific Conference Series

SP - 267

BT - New Quests in Stellar Astrophysics III: A Panchromatic View of Solar-Like Stars, With and Without Planets

A2 - Chavez, M.

A2 - Bertone, E.

A2 - Vega, O.

A2 - De la Luz, V.

PB - Publications of the Astronomical Society of the Pacific

ER -

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