Gas Motion Study of Lyα Emitters at z∼ 2 Using FUV and Optical Spectral Lines
T Hashimoto, M Ouchi, K Shimasaku… - The Astrophysical …, 2013 - iopscience.iop.org
We present the results of Magellan/MMIRS and Keck/NIRSPEC spectroscopy for five Lyα
emitters (LAEs) at z≃ 2.2 for which high-resolution FUV spectra from Magellan/MagE are
available. We detect nebular emission lines including Hα on the individual basis and low-
ionization interstellar (LIS) absorption lines in a stacked FUV spectrum, and measure
average offset velocities of the Lyα line, Δv Lyα, and LIS absorption lines, Δv abs, with
respect to the systemic velocity defined by the nebular lines. For a sample of eight z∼ 2–3 …
emitters (LAEs) at z≃ 2.2 for which high-resolution FUV spectra from Magellan/MagE are
available. We detect nebular emission lines including Hα on the individual basis and low-
ionization interstellar (LIS) absorption lines in a stacked FUV spectrum, and measure
average offset velocities of the Lyα line, Δv Lyα, and LIS absorption lines, Δv abs, with
respect to the systemic velocity defined by the nebular lines. For a sample of eight z∼ 2–3 …
Gas Motion Study of Lya Emitters at z~ 2 Using UV and Optical Spectral Lines
T Hashimoto, M Ouchi, K Shimasaku, Y Ono… - arXiv preprint arXiv …, 2012 - arxiv.org
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 …
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 …
以上显示的是最相近的搜索结果。 查看全部搜索结果