Inferring the HII region escape fraction of ionizing photons from infrared emission lines in metal-poor star-forming dwarf galaxies
نویسندگان
چکیده
Local metal-poor galaxies stand as ideal laboratories for probing the properties of interstellar medium (ISM) in chemically unevolved conditions. Detailed studies this primitive ISM can help gain insights into physics first primordial that may be responsible reionization. Quantifying porosity to ionizing photons nearby improve our understanding mechanisms leading Lyman continuum photon leakage from galaxies. The wealth infrared (IR) tracers available local and arising different phases allows us constrain complex models order estimate physical quantities.
منابع مشابه
Infrared Properties of Star Forming Dwarf Galaxies : II . Blue Compact Dwarf Galaxies in the Virgo Cluster
A sample of 16 blue compact dwarf galaxies (BCDs) in the Virgo Cluster has been imaged in the near-infrared (NIR) in J and K s on the 2.1m telescope at OAN-SPM in Mexico. Isophotes as faint as µ J = 24 mag arcsec −2 and µ Ks = 23 mag arcsec −2 have been reached in most of the targets. Surface brightness profiles can be fitted across the whole range of radii by the sum of two components: a hyper...
متن کاملStar-forming Dwarf Galaxies: Ariadne’s Thread in the Cosmic Labyrinth Star Formation in Hii Galaxies. Properties of the ionized gas
We present two set of high signal-to-noise spectrophotometric observations of three and seven compact and luminous Hii galaxies observed with the WHT and the 3.5 m telescope at CAHA, respectively. All the observations have been made with the use of a double-arm spectrograph which provides spectra with a wide wavelength coverage, from 3200 to 10500 Åfor the WHT data and 3400 to 10400 Åfor the CA...
متن کاملIonizing Photon Escape Fractions from High Redshift Dwarf Galaxies
It has been argued that low-luminosity dwarf galaxies are the dominant source of ionizing radiation during cosmological reionization. The fraction of ionizing radiation that escapes into the intergalactic medium from dwarf galaxies with masses less than ∼10 solar masses plays a critical role during this epoch. Using an extensive suite of very high resolution (0.1 pc), adaptive mesh refinement, ...
متن کاملForming a Primordial Star in a Relic Hii Region
There has been considerable theoretical debate over whether photoionization and supernova feedback from the first Population III stars facilitate or suppress the formation of the next generation of stars. We present results from an Eulerian adaptive mesh refinement simulation demonstrating the formation of a primordial star within a region ionized by an earlier nearby star. Despite the higher t...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
ژورنال
عنوان ژورنال: Astronomy and Astrophysics
سال: 2022
ISSN: ['0004-6361', '1432-0746']
DOI: https://doi.org/10.1051/0004-6361/202243866