The effect of the environment-dependent stellar initial mass function on the photometric properties of star-forming galaxies

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F24%3A10493637" target="_blank" >RIV/00216208:11320/24:10493637 - isvavai.cz</a>

Result on the web

<a href="https://verso.is.cuni.cz/pub/verso.fpl?fname=obd_publikace_handle&handle=g9eiJOPoBy" target="_blank" >https://verso.is.cuni.cz/pub/verso.fpl?fname=obd_publikace_handle&handle=g9eiJOPoBy</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1051/0004-6361/202347928" target="_blank" >10.1051/0004-6361/202347928</a>

Result language

angličtina

Original language name

The effect of the environment-dependent stellar initial mass function on the photometric properties of star-forming galaxies

Original language description

Context. Observational estimates of galaxy properties, including mass and star formation rates (SFRs), rely on the inherent galaxy-wide initial mass function (gwIMF), which systematically varies with the global SFR and metallicity, as proposed by the integrated-galactic IMF (IGIMF) theory and supported by empirical evidence. Aims. We aim to evaluate the influence of the variable gwIMF on various galaxy properties, encompassing the Ks-, K3.6-, and V-band stellar mass-to-light ratio, SFR-luminosity relation, gas depletion timescale, and stellar mass buildup timescale of local star-forming galaxies. Methods. We incorporate PARSEC and COLIBRI stellar isochrones into the GalIMF code, a galaxy chemical evolution (GCE) model featuring real-time updates of environment-dependent gwIMFs. This newly developed photometric GalIMF (photGalIMF) code allows the calculation of photometric properties for galaxies with diverse stellar populations. Subsequently, we analyze observed luminosities and metallicities of local star-forming galaxies to deduce their stellar masses assuming empirically-motivated SFHs of Local Cosmological Volume galaxies. We also compute SFR-H alpha luminosity relations for varying stellar metallicities using a separate stellar population synthesis code based on PEGASE. Results. Comparing the IGIMF theory to the canonical universal IMF, our analysis reveals that estimates of the stellar masses and SFRs for local star-forming galaxies differ by factors of approximately 2 and 10, respectively. This disparity yields a well-defined galaxy main sequence extending to dwarf galaxies. The computed gas-depletion timescale increases with gas mass, implying lower star formation efficiencies in more massive galaxies, possibly due to stronger feedback regulation, aligning with theoretical expectations. Additionally, the characteristic stellar mass buildup timescale increases with stellar mass, indicating that massive disk galaxies initiate star formation earlier than their low-mass counterparts. Conclusions. The photGalIMF code enables self-consistent computations of galactic photometry with GCE modelling adopting an environment-dependent gwIMF. Utilizing K-band and H alpha luminosities of galaxies, the outcomes include galaxy mass, SFR, and fitting functions for the SFR correction factor.

Czech name

—

Czech description

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Type

J_imp - Article in a specialist periodical, which is included in the Web of Science database

CEP classification

—

OECD FORD branch

10308 - Astronomy (including astrophysics,space science)

Project

—

Continuities

I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year

2024

Confidentiality

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Name of the periodical

Astronomy &amp; Astrophysics

ISSN

0004-6361

e-ISSN

1432-0746

Volume of the periodical

689

Issue of the periodical within the volume

září

Country of publishing house

FR - FRANCE

Number of pages

18

Pages from-to

A221

UT code for WoS article

001322521400040

EID of the result in the Scopus database

2-s2.0-85204283216