Understanding galaxy evolution through emission lines
LJ Kewley, DC Nicholls… - Annual Review of …, 2019 - annualreviews.org
We review the use of emission lines for understanding galaxy evolution, focusing on
excitation source, metallicity, ionization parameter, ISM pressure, and electron density. We …
excitation source, metallicity, ionization parameter, ISM pressure, and electron density. We …
De re metallica: the cosmic chemical evolution of galaxies
R Maiolino, F Mannucci - The Astronomy and Astrophysics Review, 2019 - Springer
The evolution of the content of heavy elements in galaxies, the relative chemical
abundances, their spatial distribution, and how these scale with various galactic properties …
abundances, their spatial distribution, and how these scale with various galactic properties …
GASP. I. Gas stripping phenomena in galaxies with MUSE
Abstract GAs Stripping Phenomena in galaxies with MUSE (GASP) is a new integral-field
spectroscopic survey with MUSE at the VLT aimed at studying gas removal processes in …
spectroscopic survey with MUSE at the VLT aimed at studying gas removal processes in …
BAT AGN spectroscopic survey. I. Spectral measurements, derived quantities, and AGN demographics
We present the first catalog and data release of the Swift-BAT AGN Spectroscopic Survey.
We analyze optical spectra of the majority of the detected AGNs (77%, 642/836) based on …
We analyze optical spectra of the majority of the detected AGNs (77%, 642/836) based on …
The PHANGS–MUSE nebular catalogue
B Groves, K Kreckel, F Santoro… - Monthly Notices of …, 2023 - academic.oup.com
Ionized nebulae provide critical insights into the conditions of the interstellar medium (ISM).
Their bright emission lines enable the measurement of physical properties, such as the gas …
Their bright emission lines enable the measurement of physical properties, such as the gas …
Theoretical evolution of optical strong lines across cosmic time
We use the chemical evolution predictions of cosmological hydrodynamic simulations with
our latest theoretical stellar population synthesis, photoionization, and shock models to …
our latest theoretical stellar population synthesis, photoionization, and shock models to …
The physical properties of star-forming galaxies in the low-redshift Universe
J Brinchmann, S Charlot, SDM White… - Monthly notices of …, 2004 - academic.oup.com
We present a comprehensive study of the physical properties of∼ 105 galaxies with
measurable star formation in the Sloan Digital Sky Survey (SDSS). By comparing physical …
measurable star formation in the Sloan Digital Sky Survey (SDSS). By comparing physical …
Theoretical modeling of starburst galaxies
We have modeled a large sample of infrared starburst galaxies using both the PEGASE v2.
0 and STARBURST99 codes to generate the spectral energy distribution (SED) of the young …
0 and STARBURST99 codes to generate the spectral energy distribution (SED) of the young …
Dust-corrected star formation rates of galaxies. II. Combinations of ultraviolet and infrared tracers
CN Hao, RC Kennicutt, BD Johnson… - The Astrophysical …, 2011 - iopscience.iop.org
We present new calibrations of far-ultraviolet (FUV) attenuation as derived from the total
infrared to FUV luminosity ratio (IRX) and the FUV–near-UV (NUV) color. We find that the …
infrared to FUV luminosity ratio (IRX) and the FUV–near-UV (NUV) color. We find that the …
The host galaxies and classification of active galactic nuclei
LJ Kewley, B Groves, G Kauffmann… - Monthly Notices of the …, 2006 - academic.oup.com
We present an analysis of the host properties of 85 224 emission-line galaxies selected from
the Sloan Digital Sky Survey. We show that Seyferts and low-ionization narrow emission-line …
the Sloan Digital Sky Survey. We show that Seyferts and low-ionization narrow emission-line …