Gaia-ESO Survey: Gas dynamics in the Carina nebula through optical emission lines

2016/04/05 by F. Damiani, R. Bonito, L. Magrini +29 · 14 citations
Physics and Astronomy · #Astronomical spectroscopy #Astronomy and Astrophysical Research #Astrophysics and Star Formation Studies #Balmer series #Dynamics (music) #Emission nebula #Emission spectrum #Gas dynamics #Nebula #O-type star #Stellar, planetary, and galactic studies #Thermal emission #astro-ph.GA #astro-ph.SR

paper · pdf · doi:10.1051/0004-6361/201628169

published in Astronomy and Astrophysics 591, A74 (EDP Sciences) · 25 pages, 42 figures, accepted for publication in Astronomy and Astrophysics

arxiv created 2016/04/05 · openalex publication_date 2016/04/20 · arxiv updated 2016/06/22 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Aims. We present observations from the Gaia-ESO Survey in the lines of Hα, [N II], [S II], and He I of nebular emission in the central part of the Carina nebula.

Citations

• High‐Mass Cloud Cores in the η Carinae Giant Molecular Cloud
• An X-ray survey of low-mass stars in Trumpler 16 with Chandra

Cited by

• TheGaia-ESO Survey: double-, triple-, and quadruple-line spectroscopic binary candidates