Systematic Non-LTE study of the −2.6 ≤ [Fe/H] ≤ 0.2 F and G dwarfs in the solar 
neighborhood - I. Stellar atmosphere parameters

Sitnova, T.; Zhao, G.; Mashonkina, L.; Chen, Y.; Liu, F.; Pakhomov, Yu.; Tan, K.; Bolte, M.; Alexeeva, S.; Grupp, F.

doi:10.1088/0004-637X/808/2/148

Item

ITEM ACTIONSEXPORT

Add to Basket

Local TagsRelease HistoryDetailsSummary

Released

Journal Article

Systematic Non-LTE study of the −2.6 ≤ [Fe/H] ≤ 0.2 F and G dwarfs in the solar neighborhood - I. Stellar atmosphere parameters

MPS-Authors

/persons/resource/persons23147

Grupp, F.
Optical and Interpretative Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

External Resource

No external resources are shared

Fulltext (restricted access)

There are currently no full texts shared for your IP range.

Fulltext (public)

There are no public fulltexts stored in PuRe

Supplementary Material (public)

There is no public supplementary material available

Citation

Sitnova, T., Zhao, G., Mashonkina, L., Chen, Y., Liu, F., Pakhomov, Y., et al. (2015). Systematic Non-LTE study of the −2.6 ≤ [Fe/H] ≤ 0.2 F and G dwarfs in the solar neighborhood - I. Stellar atmosphere parameters. The Astrophysical Journal, 808(2): 148, pp. 1-17. doi:10.1088/0004-637X/808/2/148.

Cite as: https://hdl.handle.net/11858/00-001M-0000-002A-1C9C-D

Abstract

There is no abstract available