activity
20062026
most citedOn the axisymmetric thin disk model of flattened galaxies

14 citations · 112 across the 25 of their papers we have counts for

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11 papers · 1 filter

astro-ph.GA2026

Magnetic contribution to outer-disk rotation in the spiral galaxy NGC 5055

Natalia Woźniak, Joanna Jałocha, Łukasz Bratek +1

We test whether fields of galactic strength enhance NGC~5055's outer gas rotation. Finite analytic disk decompositions yield consistent rotation--density pairs and a blended gravit…

astro-ph.GA2016★ 1 cited

Magnetic flux density from the relative circular motion of stars and partially ionized gas in the Galaxy mid-plane vicinity

Joanna Jałocha, Łukasz Bratek, Jan Pękala +2

Observations suggest a slower stellar rotation relative to gas rotation in the outer part of the Milky Way Galaxy. This difference could be attributed to an interaction with the in…

astro-ph.GA2015

Velocity dispersion as a factor modifying the distribution of mass in disk-like galaxies -- an example of galaxy UGC 6446

Szymon Sikora, Łukasz Bratek, Joanna Jałocha +1

Within the disk model framework used to approximately describe flattened galaxies, we develop an iterative method of determining column mass density from rotation curve supplemente…

astro-ph.GA2014★ 2 cited

Velocity-density twin transforms in thin disk model

Łukasz Bratek, Szymon Sikora, Joanna Jałocha +1

Ring mass density and the corresponding circular velocity in thin disk model are known to be integral transforms of one another. But it may be less familiar that the transforms can…

astro-ph.GA2014★ 1 cited

Motion of halo compact objects in the gravitational potential of a low-mass model of the Galaxy

Szymon Sikora, Łukasz Bratek, Joanna Jałocha +1

Recently, we determined a lower bound for the Milky Way mass in a point mass approximation. This result was obtained for most general spherically symmetric phase-space distribution…

astro-ph.GA2014★ 8 cited

Constraining the vertical structure of the Milky Way rotation by microlensing in a finite-width global disk model

Joanna Jałocha, Szymon Sikora, Łukasz Bratek +1

In this paper we model the vertical structure of mass distribution of the Milky Way galaxy in the framework of a finite-width global disk model. Assuming the Galactic rotation curv…

astro-ph.GA2011★ 10 cited

The role of large-scale magnetic fields in galaxy NGC 891. Can magnetic fields help to reduce the local mass-to-light ratio in the galactic outskirts?

Joanna Jałocha, Łukasz Bratek, Jan Pȩkala +1

We address the problem of the influence of large-scale magnetic fields on galactic rotation for the example of the spiral galaxy NGC 891. Based on its rotation curve and the surfac…

astro-ph.GA2011★ 3 cited

A lower bound on the Milky Way mass from general phase-space distribution function models

Łukasz Bratek, Szymon Sikora, Joanna Jałocha +1

We model the phase-space of the kinematic tracers using general, smooth distribution functions to derive a conservative lower bound on the total mass within 150-200 kpc. By approxi…

astro-ph.GA2011★ 14 cited

Gravitational microlensing as a test of a finite-width disk model of the Galaxy

Szymon Sikora, Łukasz Bratek, Joanna Jałocha +1

The aim of this work is to show, in the framework of a simple finite-width disk model, that the amount of mass seen through gravitational microlensing measurements in the region $0…

astro-ph.GA2010★ 6 cited

Vertical gradients of azimuthal velocity in a global thin disk model of spiral galaxies NGC 2403, NGC 4559, NGC 4302 and NGC 5775

Joanna Jałocha, Łukasz Bratek, Marek Kutschera +1

We estimate the vertical gradient of rotational velocity for several spiral galaxies in the framework of a global thin-disc model, using the approximation of quasi-circular orbits.…

astro-ph.GA2010★ 12 cited

Transverse gradients of azimuthal velocity in a global disk model of the Milky Way

Joanna Jałocha, Łukasz Bratek, Marek Kutschera +1

In this paper, we aim to estimate the vertical gradients in the rotational velocity of the Galaxy. This is carried out in the framework of a global thin disc model approximation. T…