The Effective Temperatures and Physical Properties of Magellanic Cloud Red Supergiants: The Effects of Metallicity

Emily M. Levesque, Philip Massey, K. A. G. Olsen, Bertrand Plez, Georges Meynet, Andre Maeder

Open source

DOI: 10.1086/504417
Published: 2006-07-10
Container: The Astrophysical Journal
Publisher: American Astronomical Society
Open access: unknown

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Cite this work

BibTeX

@article{allodium:10.1086/504417,
  title = {The Effective Temperatures and Physical Properties of Magellanic Cloud Red Supergiants: The Effects of Metallicity},
  author = {Emily M. Levesque and Philip Massey and K. A. G. Olsen and Bertrand Plez and Georges Meynet and Andre Maeder},
  year = {2006},
  journal = {The Astrophysical Journal},
  doi = {10.1086/504417},
  url = {https://doi.org/10.1086/504417}
}

RIS

TY  - JOUR
TI  - The Effective Temperatures and Physical Properties of Magellanic Cloud Red Supergiants: The Effects of Metallicity
AU  - Emily M. Levesque
AU  - Philip Massey
AU  - K. A. G. Olsen
AU  - Bertrand Plez
AU  - Georges Meynet
AU  - Andre Maeder
PY  - 2006
JO  - The Astrophysical Journal
DO  - 10.1086/504417
UR  - https://doi.org/10.1086/504417
ER  -

APA

Levesque, E. M., Massey, P., Olsen, K. A. G., Plez, B., Meynet, G., & Maeder, A. (2006). The Effective Temperatures and Physical Properties of Magellanic Cloud Red Supergiants: The Effects of Metallicity. The Astrophysical Journal. https://doi.org/10.1086/504417

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crossref · retrieved 2026-09-24T22:42:54.725Z