Lyman-alpha spectral properties of five newly discovered Lyman continuum emitters
Identifikátory výsledku
Kód výsledku v IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F17%3A00484656" target="_blank" >RIV/67985815:_____/17:00484656 - isvavai.cz</a>
Výsledek na webu
<a href="http://dx.doi.org/10.1051/0004-6361/201629264" target="_blank" >http://dx.doi.org/10.1051/0004-6361/201629264</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/0004-6361/201629264" target="_blank" >10.1051/0004-6361/201629264</a>
Alternativní jazyky
Jazyk výsledku
angličtina
Název v původním jazyce
Lyman-alpha spectral properties of five newly discovered Lyman continuum emitters
Popis výsledku v původním jazyce
We have recently reported the discovery of five low redshift Lyman continuum (LyC) emitters (LCEs) with absolute escape lfractions f(esc)(LyC) that range from 6 to 13%, higher than previously found and that more than double the number of low redshift LCEs. We use these observations to test theoretical predictions about a link between the characteristics of the Lyman-alpha (Ly alpha) line from galaxies and the escape of ionizing photons. Our LCEs are found to be strong Ly alpha emitters, with high equivalent widths, EW(Ly alpha) > 70 angstrom, and large Ly alpha escape fractions, f(esc)(Ly alpha)> 20%. The Ly alpha profiles are all double-peaked with a small peak separation, in agreement with our theoretical expectations. They also have no underlying absorption at the Ly alpha position. All these characteristics are very different from the Ly alpha properties of typical star-forming galaxies of the local Universe. A subset of the comparison samples (2-3 Green Pea galaxies) share these extreme values, indicating that they could also be leaking. We also find a strong correlation between the star formation rate surface density and the escape fraction of ionizing photons, indicating that the compactness of star-forming regions plays a role in shaping low column density paths in the interstellar medium of LCEs.
Název v anglickém jazyce
Lyman-alpha spectral properties of five newly discovered Lyman continuum emitters
Popis výsledku anglicky
We have recently reported the discovery of five low redshift Lyman continuum (LyC) emitters (LCEs) with absolute escape lfractions f(esc)(LyC) that range from 6 to 13%, higher than previously found and that more than double the number of low redshift LCEs. We use these observations to test theoretical predictions about a link between the characteristics of the Lyman-alpha (Ly alpha) line from galaxies and the escape of ionizing photons. Our LCEs are found to be strong Ly alpha emitters, with high equivalent widths, EW(Ly alpha) > 70 angstrom, and large Ly alpha escape fractions, f(esc)(Ly alpha)> 20%. The Ly alpha profiles are all double-peaked with a small peak separation, in agreement with our theoretical expectations. They also have no underlying absorption at the Ly alpha position. All these characteristics are very different from the Ly alpha properties of typical star-forming galaxies of the local Universe. A subset of the comparison samples (2-3 Green Pea galaxies) share these extreme values, indicating that they could also be leaking. We also find a strong correlation between the star formation rate surface density and the escape fraction of ionizing photons, indicating that the compactness of star-forming regions plays a role in shaping low column density paths in the interstellar medium of LCEs.
Klasifikace
Druh
J<sub>imp</sub> - Článek v periodiku v databázi Web of Science
CEP obor
—
OECD FORD obor
10308 - Astronomy (including astrophysics,space science)
Návaznosti výsledku
Projekt
<a href="/cs/project/GP14-20666P" target="_blank" >GP14-20666P: Původ emise a absorpce Lyman alfa v galaxiích</a><br>
Návaznosti
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)
Ostatní
Rok uplatnění
2017
Kód důvěrnosti údajů
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Údaje specifické pro druh výsledku
Název periodika
Astronomy & Astrophysics
ISSN
1432-0746
e-ISSN
—
Svazek periodika
597
Číslo periodika v rámci svazku
January
Stát vydavatele periodika
FR - Francouzská republika
Počet stran výsledku
13
Strana od-do
"A13/1"-"A13/13"
Kód UT WoS článku
000392392900098
EID výsledku v databázi Scopus
2-s2.0-85007246530