Stellar and wind properties of massive stars in the central parsec of the Galaxy

0Citations
Citations of this article
9Readers
Mendeley users who have this article in their library.

Abstract

The stellar and wind properties of the new population of massive stars in the central parsec of the Galaxy are derived through quantitative analysis with atmosphere models. © 2007 International Astronomical Union.

Cite

CITATION STYLE

APA

Martins, F., Genzel, R., Eisenhauer, F., Paumard, T., Ott, T., Trippe, S., & Gillessen, S. (2006). Stellar and wind properties of massive stars in the central parsec of the Galaxy. In Proceedings of the International Astronomical Union (Vol. 2, p. 207). Cambridge University Press. https://doi.org/10.1017/S1743921307010198

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free