Gas Motion Study of Lya Emitters at z~2 Using UV and Optical Spectral Lines
arXiv:1206.2316 · doi:10.1088/0004-637X/765/1/70
Abstract
We present the results of Magellan/MMIRS and Keck/NIRSPEC spectroscopy for five Lya emitters (LAEs) at z=2.2 for which high-resolution FUV spectra from Magellan/MagE are available. We detect nebular emission lines including Ha on the individual basis and low-ionization interstellar (LIS) absorption lines in a stacked FUV spectrum, and measure average offset velocities of the Lya line, Delta_v_Lya, and LIS absorption lines, Delta_v_abs, with respect to the systemic velocity defined by the nebular lines. For a sample of eight z~2-3 LAEs without AGN from our study and the literature, we obtain Delta_v_Lya = 175+/-35 km s^{-1}, which is significantly smaller than that of Lyman-break Galaxies (LBGs), Delta_v_Lya=400 km s^{-1}. The stacked FUV spectrum gives Delta_v_abs = -179 +/- 73 km s^{-1}, comparable to that of LBGs. These positive Delta_v_Lya and negative Delta_v_abs suggest that LAEs also have outflows. In contrast to LBGs, however, the LAEs' Delta_v_Lya is as small as |Delta_v_abs|, suggesting low neutral hydrogen column densities. Such a low column density with a small number of resonant scattering may cause the observed strong Lya emission of LAEs. We find an anti-correlation between Lya equivalent width (EW) and Delta_v_Lya in a compilation of LAE and LBG samples. Although its physical origin is not clear, this anti-correlation result appears to challenge the hypothesis that a strong outflow, by means of a reduced number of resonant scattering, produces a large EW. If LAEs at z>6 have similarly small Delta_v_Lya values, constraints on the reionization history derived from the Lya transmissivity may need to be revised.
15 pages, 13 figures, 7 tables. Accepted for publication in ApJ
References in corpus (17)
- Cold streams in early massive hot haloes as the main mode of galaxy formation
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Likelihoods and Parameters from the WMAP data
- The Mass-Metallicity Relation at z~2
- The Stellar, Gas and Dynamical Masses of Star-Forming Galaxies at z~2
- 3D Lyman-alpha radiation transfer. I. Understanding Lyman-alpha line profile morphologies
- The Chandra COSMOS Survey, I: Overview and Point Source Catalog
- Multi-Wavelength Constraints on the Cosmic Star Formation History from Spectroscopy: the Rest-Frame UV, H-alpha, and Infrared Luminosity Functions at Redshifts 1.9<z<3.4
- The End of the Reionization Epoch Probed by Ly-alpha Emitters at z=6.5 in the Subaru Deep Field
- The Multiwavelength Survey by Yale-Chile (MUSYC): Deep Medium-Band optical imaging and high quality 32-band photometric redshifts in the ECDF-S
- A Population of Faint Extended Line Emitters and the Host Galaxies of Optically Thick QSO Absorption Systems
- 3D Lyman-alpha radiation transfer. III. Constraints on gas and stellar properties of z~3 Lyman break galaxies (LBG) and implications for high-z LBGs and Lyman-alpha emitters(LAEs)
- The Properties and Prevalence of Galactic Outflows at z = 1 in the Extended Groth Strip
- On the Detectability of Lyman-alpha Emission in Star-forming Galaxies: The Role of Dust
- Effects of Dust Geometry in Lyman Alpha Galaxies at z = 4.4
- Turning Back the Clock: Inferring the History of the Eight O'clock Arc
- The Optically Unbiased GRB Host (TOUGH) survey. IV. Lyman-alpha emitters
- Intrinsic Shape of Star-Forming BzK Galaxies II: Rest-Frame UV and Optical Structures in GOODS-South and SXDS
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- Lyα Equivalent Width Distribution of Lyα Emitting Galaxies at Redshift z 4.5
- The MUSE Hubble Ultra Deep Field Survey. XV. The mean rest-UV spectra of Ly-alpha emitters at z>3
- Lyman-Alpha Emitter Galaxies at z ~ 2.8 in the Extended Chandra Deep Field-South: I. Tracing the Large-Scale Structure via Lyman-Alpha Imaging
- Environmental Dependence of Galactic Properties Traced by Ly Forest Absorption: Diversity among Galaxy Populations
- A new quadruple gravitational lens from the Hyper Suprime-Cam Survey: the puzzle of HSC~J115252+004733
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- Magellan/MMIRS near-infrared multi-object spectroscopy of nebular emission from star forming galaxies at 2<z<3
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