SpringerLink
Forum Springer Astron. Astrophys.
Forum Whats New Search Orders


Astron. Astrophys. 334, 11-20 (1998)

Next Section Table of Contents

HST study of Lyman-alpha emission in star-forming galaxies:
the effect of neutral gas flows *

Daniel Kunth 1, J.M. Mas-Hesse 2, E. Terlevich 3, R. Terlevich 4, J. Lequeux 5 and S. Michael Fall 6

1 Institut d'Astrophysique de Paris, 98bis Bld Arago, F-75014 Paris, France
2 LAEFF-INTA, POB 50727, E-28080 Madrid, Spain
3 Institute of Astronomy, Madingley Road, Cambridge CB3 0HA, UK
4 Royal Greenwich Observatory, Madingley Road, Cambridge CB3 0EZ, UK
5 DEMIRM, Observatoire de Paris, 61 Av. de l'Observatoire, F-75014 Paris, France
6 Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA

Received 27 October 1997 / Accepted 16 February 1998

Abstract

We present high dispersion HST GHRS UV spectroscopic observations of 8 H II galaxies covering a wide range of metallicities and physical properties. We have found Ly [FORMULA] emission in 4 galaxies with blueshifted absorption features, leading to P Cygni like profiles in 3 of them. In all these objects the O I and Si II absorption lines are also blueshifted with respect to the ionized gas, indicating that the neutral gas is outflowing in these galaxies with velocities up to 200 km s-1 or more. The rest of the sample shows broad damped Ly [FORMULA] absorption profiles centered at the wavelength corresponding to the redshift of the H II emitting gas. We therefore find that the velocity structure of the neutral gas in these galaxies is the driving factor that determines the detectability of Ly [FORMULA] in emission. Relatively small column densities of neutral gas with even very small dust content would destroy the Ly [FORMULA] emission if this gas is static with respect to the ionized region where Ly [FORMULA] photons originate. The situation changes dramatically when most of the neutral gas is velocity-shifted with respect to the ionized regions because resonant scattering by neutral hydrogen will be most efficient at wavelengths shorter than the Ly [FORMULA] emission, allowing the Ly [FORMULA] photons to escape (at least partially). This mechanism complements the effect of porosity in the neutral interstellar medium discussed by other authors, which allows to explain the escape of Ly [FORMULA] photons in regions surrounded by static neutral gas, but with only partial covering factors. The anisotropy of these gas flows and their dependence on the intrinsic properties of the violent star-forming episodes taking place in these objects (age, strength, gas geometry,...) might explain (in part) the apparent lack of correlation between other properties (like metallicity) and the frequency of occurence and strength of Ly [FORMULA] emission in star-forming galaxies. Attempts to derive the comoving star-formation rate at high redshifts from Ly [FORMULA] emission searches are highly questionable.

Key words: galaxies: ISM – galaxies: irregular – galaxies: compact – galaxies: starbust – cosmology: observations – ultraviolet: galaxies

* Based on observations with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract No. NAS5-26555.

Send offprint requests to: D. Kunth (IAP address), (kunth@iap.fr)

SIMBAD Objects

Contents

Next Section Table of Contents

© European Southern Observatory (ESO) 1998

Online publication: May 12, 1998

helpdesk.link@springer.de