Zobrazeno 1 - 10
of 286
pro vyhledávání: '"Vukotić B."'
Recent studies of Galactic evolution revealed that the dynamics of the stellar component might be one of the key factors when considering galactic habitability. We run an N-body simulation model of the Milky Way, which we evolve for 10 Gyr, to study
Externí odkaz:
http://arxiv.org/abs/2310.16227
Publikováno v:
Serbian Astronomical Journal, 2019, volume 199
In this paper we present the updated empirical radio surface-brightness-to-diameter ($\Sigma$--$D$) relation for Galactic supernova remnants (SNRs) calibrated using $110$ SNRs with reliable distances. We apply orthogonal fitting procedure and kernel
Externí odkaz:
http://arxiv.org/abs/1912.06379
The problem of the extent of habitable zones in different kinds of galaxies is one of the outstanding challenges for contemporary astrobiology. In the present study, we investigate habitability in a large sample of simulated galaxies from the Illustr
Externí odkaz:
http://arxiv.org/abs/1909.01742
Autor:
Maggi, P., Filipovic, M. D., Vukotic, B., Ballet, J., Haberl, F., Maitra, C., Kavanagh, P., Sasaki, M., Stupar, M.
Publikováno v:
A&A 631, A127 (2019)
Aims: We present a comprehensive study of the supernova remnant (SNR) population of the Small Magellanic Cloud (SMC). We measure multiwavelength properties of the SMC SNRs and compare them to those of the Large Magellanic Cloud (LMC) population. Meth
Externí odkaz:
http://arxiv.org/abs/1908.11234
Autor:
Maxted, Nigel I., Braiding, C., Wong, G. F., Rowell, G. P., Burton, M. G., Filipovic, M. D., Voisin, F., Urosevic, D., Vukotic, B., Pavlovic, M. Z., Sano, H., Fukui, Y.
The Galactic supernova remnant HESS J1534-571 (also known as G323.7-1.0) has a shell-like morphology in TeV gamma-ray emission and is a key object in the study of cosmic ray origin. Little is known about its distance and local environment. We examine
Externí odkaz:
http://arxiv.org/abs/1807.01300
We present 21 new radio-continuum detections at catalogued planetary nebula (PN) positions in the Large Magellanic Cloud (LMC) using all presently available data from the Australia Telescope Online Archive at 3, 6, 13 and 20 cm. Additionally, 11 prev
Externí odkaz:
http://arxiv.org/abs/1703.01489
Publikováno v:
MNRAS, 2016, Volume 459, Issue 4, Pp. 3512-3524
We present an isolated Milky Way-like simulation in GADGET2 N-body SPH code. The Galactic disk star formation rate (SFR) surface densities and stellar mass indicative of Solar neighbourhood are used as thresholds to model the distribution of stellar
Externí odkaz:
http://arxiv.org/abs/1604.01664
Publikováno v:
Serb. Astron. J., 189, 25 (2014)
We present updated empirical radio surface-brightness-to-diameter ($\Sigma-D$) relation for supernova remnants (SNRs) in our Galaxy. Our original calibration sample of Galactic SNRs with independently determined distances (Pavlovic et al. 2013, herea
Externí odkaz:
http://arxiv.org/abs/1411.2234
Publikováno v:
MNRAS 440, 2026-2035 (2014)
We present a method for distance calibration without using standard fitting procedures. Instead we use random resampling to reconstruct the probability density function (PDF) of calibration data points in the fitting plane. The resulting PDF is then
Externí odkaz:
http://arxiv.org/abs/1403.1368
Publikováno v:
Astrophys. J., 777, 31 (2013)
The equipartition or minimum-energy calculation is a well-known procedure for estimating magnetic field strength and total energy in the magnetic field and cosmic ray particles by using only the radio synchrotron emission. In one of our previous pape
Externí odkaz:
http://arxiv.org/abs/1308.6110