The Lyman alpha reference sample: VII. Spatially resolved H α kinematics

Edmund Christian Herenz, Pieter Gruyters, Ivana Orlitova, Matthew Hayes, Göran Östlin, John M. Cannon, Martin M. Roth, Arjan Bik, Stephen Pardy, Héctor Otí-Floranes, J. Miguel Mas-Hesse, Angela Adamo, Hakim Atek, Florent Duval, Lucia Guaita, Daniel Kunth, Peter Laursen, Jens Melinder, Johannes Puschnig, Thøger E. Rivera-ThorsenDaniel Schaerer, Anne Verhamme

Resultado de la investigación: Contribución a una revistaArtículorevisión exhaustiva

23 Citas (Scopus)

Resumen

We present integral field spectroscopic observations with the Potsdam Multi-Aperture Spectrophotometer of all 14 galaxies in the z ∼ 0.1 Lyman Alpha Reference Sample (LARS). We produce 2D line-of-sight velocity maps and velocity dispersion maps from the Balmer α (Hα) emission in our data cubes. These maps trace the spectral and spatial properties of the LARS galaxies' intrinsic Lyα radiation field. We show our kinematic maps that are spatially registered onto the Hubble Space Telescope Hα and Lyman α (Lyα) images. We can conjecture a causal connection between spatially resolved Hα kinematics and Lyα photometry for individual galaxies, however, no general trend can be established for the whole sample. Furthermore, we compute the intrinsic velocity dispersion σ0, the shearing velocity νshear, and the νshear0 ratio from our kinematic maps. In general LARS galaxies are characterised by high intrinsic velocity dispersions (54 km s-1 median) and low shearing velocities (65 km s-1 median). The νshear0 values range from 0.5 to 3.2 with an average of 1.5. It is noteworthy that five galaxies of the sample are dispersion-dominated systems with νshear0< 1, and are thus kinematically similar to turbulent star-forming galaxies seen at high redshift. When linking our kinematical statistics to the global LARS Lyα properties, we find that dispersion-dominated systems show higher Lyα equivalent widths and higher Lyα escape fractions than systems with νshear0> 1. Our result indicates that turbulence in actively star-forming systems is causally connected to interstellar medium conditions that favour an escape of Lyα radiation.

Idioma originalInglés
Número de artículoA78
PublicaciónAstronomy and Astrophysics
Volumen587
DOI
EstadoPublicada - 1 mar 2016
Publicado de forma externa

Áreas temáticas de ASJC Scopus

  • Astronomía y astrofísica
  • Ciencias planetarias y espacial

Huella

Profundice en los temas de investigación de 'The Lyman alpha reference sample: VII. Spatially resolved H α kinematics'. En conjunto forman una huella única.

Citar esto