Correlation between star formation activity and electron density of ionized gas at z = 2.5 | Zendy

Rhythm Shimakawa | Zendy; Tadayuki Kodama | Zendy; Charles C. Steidel | Zendy; Ken-ichi Tadaki | Zendy; Ichi Tanaka | Zendy; Allison L. Strom | Zendy; Masao Hayashi | Zendy; Yusei Koyama | Zendy; Tomoko L. Suzuki | Zendy; Moegi Yamamoto | Zendy

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Correlation between star formation activity and electron density of ionized gas at z = 2.5

Author(s) -

Rhythm Shimakawa,

Tadayuki Kodama,

Charles C. Steidel,

Ken-ichi Tadaki,

Ichi Tanaka,

Allison L. Strom,

Masao Hayashi,

Yusei Koyama,

Tomoko L. Suzuki,

Moegi Yamamoto

Publication year - 2015

Publication title -

monthly notices of the royal astronomical society

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 2.058

H-Index - 383

eISSN - 1365-8711

pISSN - 0035-8711

DOI - 10.1093/mnras/stv915

Subject(s) - physics , astrophysics , galaxy , star formation , redshift , interstellar medium , ionization , electron density , electron , ion , quantum mechanics

In the redshift interval of 2 < z < 3, the physical conditions of the interstellar medium (ISM) in star-forming galaxies are likely to be different from those in the local Universebecause of lower gaseous metallicities, higher gas fractions, and higher star formation activities. In fact, observations suggest that higher electron densities, higher ionization parameters, and harder UV radiation fiel...

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