2020A&A...639A..85G


Query : 2020A&A...639A..85G

2020A&A...639A..85G - Astronomy and Astrophysics, volume 639A85-85 (2020/7-1)

The origin of the escape of Lyman α and ionizing photons in Lyman continuum emitters.

GAZAGNES S., CHISHOLM J., SCHAERER D., VERHAMME A. and IZOTOV Y.

Abstract (from CDS):


Context.Identifying the physical mechanisms driving the escape of Lyman continuum (LyC) photons is crucial for the search of Lyman continuum emitter (LCE) candidates.
Aims. To understand the physical properties involved in the leakage of LyC photons, we investigate the connection between the HI covering fraction, HI velocity width, the Lyman α (Lyα) properties, and the escape of LyC photons in a sample of 22 star-forming galaxies, which includes 13 confirmed LCEs.
Methods. We fit the stellar continuum, dust attenuation, and absorption lines between 920Å and 1300Å to extract the HI covering fractions and dust attenuation. Additionally, we measure the HI velocity widths of the optically thick Lyman series and derive the Lyα equivalent widths (EW), escape fractions (fesc), peak velocities, and fluxes at the minimum of the observed Lyα profiles.
Results. Overall, we highlight strong observational correlations between the presence of low HI covering fractions and the observation of (1) low Lyα peak velocities; (2) more flux at the profile minimum; and (3) larger EW(Lyα), fesc(Lyα), and fescobs(LyC). Hence, low column density channels are crucialISM ingredients for the leakage of Lyα and LyC photons. Additionally, galaxies with narrower HI absorption velocity widths have higher Lyα equivalent widths, larger Lyα escape fractions, and lower Lyα peak velocity separations. This may suggest that these galaxies have low HI column density. Finally, we find that dust also regulates the amount of Lyα and LyC radiation that actually escapes theISM.
Conclusions. TheISM porosity is one of the origins of strong Lyα emission, enabling the escape of ionizing photons in low-z leakers. However, this is not sufficient to explain the largest fescobs(LyC), which indicates that the most extreme LCEs are likely to be density-bounded along all lines of sight to the observer. Overall, the neutral gas porosity provides a constraint for a lower limit to the escape fraction of LyC and Lyα photons, which offers a key estimator for assessing the leakage of ionizing photons.

Abstract Copyright: © ESO 2020

Journal keyword(s): dark ages, reionization, first stars - galaxies: ISM - ultraviolet: ISM - ISM: abundances - ISM: lines and bands - dust, extinction

Simbad objects: 26

goto Full paper

goto View the references in ADS

Number of rows : 26
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NAME SMC G 00 52 38.0 -72 48 01   2.79 2.2     ~ 12317 1
2 SHOC 148 Sy1 03 03 21.4159312248 -07 59 23.230161564     19.61     ~ 35 0
3 2MASX J04420810-3801108 H2G 04 42 08.110 -38 01 10.88 15.66 17.21 15.80 16.00   ~ 54 0
4 SDSS J090145.62+211927.7 G 09 01 45.62088 +21 19 27.7824           ~ 15 0
5 SDSS J091113.34+183108.1 EmG 09 11 13.3468379280 +18 31 08.213614176           ~ 33 0
6 2MASS J09215939+4509126 QSO 09 21 59.397 +45 09 12.38   18.57 18.31     ~ 64 0
7 SDSS J092532.36+140313.1 EmG 09 25 32.3639224872 +14 03 12.998128212           ~ 39 0
8 SDSS J092600.41+442736.1 AGN 09 26 00.4038688128 +44 27 36.171019692           ~ 91 0
9 SDSS J101138.27+194720.9 G 10 11 38.2749128232 +19 47 20.905754784           ~ 18 0
10 SDSS J105330.82+523752.8 G 10 53 30.8149860768 +52 37 52.857629508           ~ 33 0
11 SDSS J115204.88+340049.8 EmG 11 52 04.8869459880 +34 00 49.917538404           ~ 28 0
12 SDSS J115448.85+244333.0 G 11 54 48.854 +24 43 33.04           ~ 31 0
13 SGAS J122651.3+215220 LeG 12 26 51.3 +21 52 20           ~ 32 0
14 SDSS J124300.62+464650.5 G 12 43 00.6331121352 +46 46 50.495845548           ~ 22 0
15 SDSS J124423.37+021540.4 EmG 12 44 23.3871660288 +02 15 40.467424356           ~ 37 0
16 SDSS J124810.48+425953.7 G 12 48 10.4839133976 +42 59 53.683847016           ~ 17 0
17 EC 12476-2317 AGN 12 50 18.90 -23 33 57.6   16.29 15.46     ~ 72 0
18 SDSS J125644.15+450917.1 G 12 56 44.15136 +45 09 17.1828           ~ 11 0
19 Z 189-2 GiC 12 56 55.638 +32 26 51.50   15.1       ~ 90 0
20 SDSS J133303.95+624603.8 H2G 13 33 03.9554834328 +62 46 03.761300964           ~ 25 0
21 [ITS2007] 53531-1827-503 EmG 14 29 47.0072305272 +06 43 34.964991264           ~ 41 0
22 SDSS J144231.37-020952.0 G 14 42 31.3701588768 -02 09 51.960248712   20.28       ~ 34 0
23 SDSS J150342.82+364450.7 EmG 15 03 42.8266534776 +36 44 50.729142300           ~ 27 0
24 [BHG2011] SDSS J1527+0652 A1 LeG 15 27 48.950 +06 52 23.09           ~ 22 0
25 SDSS J160810.36+352809.3 EmG 16 08 10.3514480208 +35 28 09.370755984           ~ 19 0
26 NAME Cosmic Eye G 21 35 12.730 -01 01 42.90           ~ 92 0

To bookmark this query, right click on this link: simbad:objects in 2020A&A...639A..85G and select 'bookmark this link' or equivalent in the popup menu