36 citations · 90 across the 10 of their papers we have counts for
10 papers
Stochastic 2-D galaxy disk evolution models. Resolved stellar populations in the galaxy M33
T. Mineikis, V. Vansevičius
We improved the stochastic 2-D galaxy disk models (Mineikis & Vansevičius 2014a) by introducing enriched gas outflows from galaxies and synthetic color-magnitude diagrams of stella…
Deriving physical parameters of unresolved star clusters IV. The M33 star cluster system
P. de Meulenaer, D. Narbutis, T. Mineikis +1
Context. When trying to derive the star cluster physical parameters of the M33 galaxy using broad-band unresolved ground-based photometry, previous studies mainly made use of simpl…
Deriving physical parameters of unresolved star clusters III. Application to M31 PHAT clusters
Philippe de Meulenaer, Donatas Narbutis, Tadas Mineikis +1
This study is the third of a series that investigates the degeneracy and stochasticity problems present in the determination of physical parameters such as age, mass, extinction, a…
Stochastic 2-D Models of Galaxy Disk Evolution. The Galaxy M33
Tadas Mineikis, Vladas Vansevičius
We have developed a fast numerical 2-D model of galaxy disk evolution (resolved along the galaxy radius and azimuth) by adopting a scheme of parameterized stochastic self-propagati…
Structural Parameters of Star Clusters: Stochastic Effects
D. Narbutis, R. Stonkutė, P. de Meulenaer +2
Stochasticity of bright stars introduces uncertainty and bias into derived structural parameters of star clusters. We have simulated a grid of cluster -band images, observed wit…
Deriving structural parameters of semi-resolved star clusters. FitClust: a program for crowded fields
D. Narbutis, D. Semionov, R. Stonkutė +4
Context. An automatic tool to derive structural parameters of semi-resolved star clusters located in crowded stellar fields in nearby galaxies is needed for homogeneous processing…
Deriving physical parameters of unresolved star clusters. II. The degeneracies of age, mass, extinction, and metallicity
Philippe de Meulenaer, Donatas Narbutis, Tadas Mineikis +1
This paper is the second of a series that investigates the stochasticity and degeneracy problems that hinder the derivation of the age, mass, extinction, and metallicity of unresol…
Stochasticity effects on derivation of physical parameters of unresolved star clusters
Philippe de Meulenaer, Donatas Narbutis, Tadas Mineikis +1
We developed a method for a fast modeling of broad-band UBVRI integrated magnitudes of unresolved star clusters and used it to derive their physical parameters (age, mass, and exti…
Deriving physical parameters of unresolved star clusters. I. Age, mass, and extinction degeneracies
Philippe de Meulenaer, Donatas Narbutis, Tadas Mineikis +1
Context. Stochasticity and physical parameter degeneracy problems complicate the derivation of the parameters (age, mass, and extinction) of unresolved star clusters when using bro…
Disk Galaxy Models Driven by Stochastic Self-Propagating Star Formation
T. Mineikis, V. Vansevičius
We present a model of chemical and spectrophotometric evolution of disk galaxies based on a stochastic self-propagating star formation scenario. The model incorporates galaxy forma…