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相关论文: On the Lyman-alpha Emission of Starburst Galaxies

200 篇论文

We review the Lyan alpha emission in local star-forming galaxies. In most cases as already shown by the IUE, the emission is absent or much weaker than expected. This occurs because Lyman alpha photons can be resonantly scattered by the…

天体物理学 · 物理学 2007-05-23 D. Kunth , E. Terlevich , R. Terlevich , G. Tenorio-Tagle

Lyman-alpha is now widely used to investigate the galaxy formation and evolution in the high redshift universe. However, without a rigorous understanding of the processes which regulate the Lya escape fraction, physical interpretations of…

天体物理学 · 物理学 2008-09-15 Hakim Atek , Daniel Kunth , Matthew Hayes , Goeran Ostlin , J. Miguel Mas-Hesse , .

We review the imaging and spectroscopic properties of the Lyman alpha emission in starburst galaxies. The Lyman alpha photons escape is largely driven by kinematical and orientation effects related to the presence of large scale expanding…

天体物理学 · 物理学 2007-05-23 Daniel Kunth , M. Hayes , G. Ostlin , J. M. Mas-Hesse , C. Leitherer , A. Petrosian

The usefulness of H I Lyman-alpha photons for characterizing star formation in the distant universe is limited by our understanding of the astrophysical processes that regulate their escape from galaxies. These processes can only be…

宇宙学与河外天体物理 · 物理学 2015-06-12 A. Wofford , C. Leitherer , J. Salzer

We present Ly $\alpha$ imaging of 45 low redshift star-forming galaxies observed with the Hubble Space Telescope. The galaxies have been selected to have moderate to high star formation rates using far-ultraviolet (FUV) luminosity and \ha…

The detection of Ly alpha emission in star-forming galaxies in different shapes and intensities (always smaller than predicted for case B recombination) has puzzled the astronomical community for more than a decade. Here we use two…

We compare the H-beta line strengths of 1.90 < z < 2.35 star-forming galaxies observed with the near-IR grism of the Hubble Space Telescope with ground-based measurements of Ly-alpha from the HETDEX Pilot Survey and narrow-band imaging. By…

HST imaging and slitless spectroscopy are used to examine where the strong Lyman alpha emission escapes from the interstellar medium in the starburst galaxy Mkn 357. An H-alpha image shows that the ionized gas is mostly in a global wind,…

天体物理学 · 物理学 2009-11-10 William C. Keel

Star forming galaxies at high redshift show ubiquitously high ionization parameters, as measured by the ratio of optical emission lines. We demonstrate that local (z < 0.2) sources selected as Lyman break analogues also manifest high line…

星系天体物理 · 物理学 2015-06-22 E. R. Stanway , J. J. Eldridge , S. M. L. Greis , L. J. M. Davies , S. M. Wilkins , M. N. Bremer

A model for gas outflows is proposed which simultaneously explains the correlations between the (i) equivalent width of low ionization and Ly-alpha lines, (ii) outflow velocity, and (iii) star formation rate observed in Lyman Break Galaxies…

天体物理学 · 物理学 2009-11-11 A. Ferrara , M. Ricotti

Blind spectroscopy of massive lensing galaxy clusters with MUSE has revealed large numbers of gravitationally-lensed Lyman-$ \alpha $ emitters exhibiting asymmetric profiles at $ 2.9 \leq z \leq 6.7 $, suggesting abundant outflows from…

星系天体物理 · 物理学 2024-10-30 James Nianias , Jeremy Lim , Yik Lok Wong , Gordon Wong , Ishika Kaur , Wenjun Chen

We have compiled a library of stellar Lyman-alpha equivalent widths in O and B stars using the model atmosphere codes CMFGEN and TLUSTY, respectively. The equivalent widths range from about 0 to 30 \AA in absorption for early-O to mid-B…

宇宙学与河外天体物理 · 物理学 2015-06-17 Maria A. Pena-Guerrero , Claus Leitherer

We present the results of a high resolution UV 2-D spectroscopic survey of star forming galaxies observed with HST-STIS. Our main aim was to map the Lyman alpha profiles to learn about the gas kinematics and its relation with the escape of…

天体物理学 · 物理学 2009-11-10 J. M. Mas-Hesse , D. Kunth , G. Tenorio-Tagle , C. Leitherer , R. J. Terlevich , E. Terlevich

A significant fraction of the high-redshift galaxies show strong Lyman emission lines. For redshifts z>5, most known galaxies belong to this class. However, so far not much is known about the physical structure and nature of these objects.…

天体物理学 · 物理学 2009-11-13 C. Tapken , I. Appenzeller , S. Noll , S. Richling , J. Heidt , E. Meinkoehn , D. Mehlert

We present the results of a photometric and spectroscopic survey of 321 Lyman break galaxies (LBGs) at z ~ 3 to investigate systematically the relationship between Lya emission and stellar populations. Lya equivalent widths (EW) were…

宇宙学与河外天体物理 · 物理学 2014-11-20 Katherine A. Kornei , Alice E. Shapley , Dawn K. Erb , Charles C. Steidel , Naveen A. Reddy , Max Pettini , Milan Bogosavljevic

We present reduced and calibrated high resolution Lyman-alpha (Lya) images for a sample of 6 local star forming galaxies. Targets were selected to represent a range in luminosity and metallicity and to include both known Lya emitters and…

During the epoch of reionisation the first galaxies were enshrouded in pristine neutral gas, with one of the brightest emission lines in star-forming galaxies, Lyman-$\alpha$ (Ly$\alpha$), expected to remain undetected until the Universe…

We report on new imaging observations of the Lyman alpha emission line (Lya), performed with the Hubble Space Telescope, that comprise the backbone of the Lyman alpha Reference Sample (LARS). We present images of 14 starburst galaxies at…

Models are presented for the Lyman alpha emission of dusty high-redshift galaxies by combining the Press-Schechter formalism with a treatment of the inhomogeneous dust distribution inside galaxies. It is found that the amount of Lyman alpha…

天体物理学 · 物理学 2008-11-26 Zoltan Haiman , Marco Spaans

We present discovery spectra of a sample of eight lensed galaxies at high redshift, 3.7<z<5.2, selected by their red colors in the fields of four massive clusters: A1689, A2219, A2390, and AC114. Metal absorption lines are detected and…

天体物理学 · 物理学 2009-11-07 Brenda Frye , Tom Broadhurst , Narciso Benitez
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