Search Publications

Orbital eccentricities as indicators of stellar populations. A kinematical analysis of the local disc from Gaia DR2 catalogue
DOI: 10.1051/0004-6361/202040017 Bibcode: 2021A&A...649A..48C

Cubarsi, R.; Stojanović, M.; Ninković, S.


Aims: Based on a local sample from Gaia DR2 catalogue composed of 74 339 stars, we are able to derive more accurate kinematic statistics defining the local stellar populations and classify the stars in terms of their planar and vertical orbital eccentricities.
Methods: Firstly, we carried out a kinematical characterisation of stellar pop…

2021 Astronomy and Astrophysics
Gaia 3
Optical counterparts of ULXs in two dwarf galaxies: NGC 4861 and NGC 4449
DOI: 10.1093/mnras/stab1321 Bibcode: 2021MNRAS.505..771O

Ozdogan Ela, M.; Akyuz, A.; Aksaker, N. +7 more

We present the results of a search for optical candidates of ultraluminous X-ray sources (ULXs) in two dwarf galaxies, NGC 4861 and NGC 4449, using Hubble Space Telescope (HST) archival data. With precise astrometry, we confirm that NGC 4861 X1 is associated with an H II complex and we conclude that NGC 4861 X2 resides in a young star group of mas…

2021 Monthly Notices of the Royal Astronomical Society
Gaia XMM-Newton eHST 3
The destruction of the cometary nucleus - The case of 73P/Schwassmann-Wachmann
DOI: 10.1016/j.newast.2021.101626 Bibcode: 2021NewA...8901626W

Wesołowski, M.

The paper presents an analysis of the actual brightness change of comet 73P/Schwassmann-Wachmann, which took place in 1995. The consequence of a cometary outburst is the destruction of a fragment of its surface. This causes the emission of comet material from both the surface and from exposed subsurface layers. Therefore, the calculations take int…

2021 New Astronomy
Rosetta 3
Partitioning the Galactic halo with Gaussian Mixture Models
DOI: 10.1088/1674-4527/21/5/128 Bibcode: 2021RAA....21..128L

Zhao, Gang; Zhao, Jing-Kun; Liang, Xi-Long +1 more

The Galactic halo is supposed to form from merging with nearby dwarf galaxies. In order to probe different components of the Galactic halo, we have applied the Gaussian Mixture Models method to a selected sample of metal poor stars with [Fe/H] < -0.7 dex in the APOGEE DR16 catalogue based on four-parameters, metallicity, [Mg/Fe] ratio and spati…

2021 Research in Astronomy and Astrophysics
Gaia 3
Evidence for Cold Plasma in Planetary Nebulae From Radio Observations With the LOw Frequency ARray (LOFAR)
DOI: 10.3847/1538-4357/ac0fda Bibcode: 2021ApJ...919..121H

White, Glenn J.; Haverkorn, Marijke; Shimwell, Timothy +6 more

We present observations of planetary nebulae with the LOw Frequency ARray (LOFAR) between 120 and 168 MHz. The images show thermal free-free emission from the nebular shells. We have determined the electron temperatures for spatially resolved, optically thick nebulae. These temperatures are 20%-60% lower than those estimated from collisionally exc…

2021 The Astrophysical Journal
Herschel eHST 3
On the unified view of extragalactic sources based on their broadband emission properties
DOI: 10.1007/s12036-021-09778-4 Bibcode: 2021JApA...42..107I

Iyida, E. U.; Eya, I. O.; Odo, F. C.

Our understanding of the unification of jetted active galactic nuclei (AGNs) has advanced greatly as the size of extragalactic sources increased. In this paper, based on the large sample of radio sources, we compiled 680 blazars (279 flat spectrum radio quasars (FSRQs) and 401 BL Lacertae (BL Lacs)) from the 3FGL sample and 64 Seyfert galaxies (3 …

2021 Journal of Astrophysics and Astronomy
INTEGRAL 3
A Gemini-NIFS view of the merger remnant NGC 34
DOI: 10.1093/mnras/stab1977 Bibcode: 2021MNRAS.506.4354M

Pastoriza, M. G.; Storchi-Bergmann, T.; Ricci, T. V. +8 more

The merger remnant NGC 34 is a local luminous infrared galaxy (LIRG) hosting a nuclear starburst and a hard X-ray source associated with a putative, obscured Seyfert 2 nucleus. In this work, we use adaptive optics assisted near-infrared (NIR) integral field unit observations of this galaxy to map the distribution and kinematics of the ionized and …

2021 Monthly Notices of the Royal Astronomical Society
eHST 3
The sharpest ultraviolet view of the star formation in an extreme environment of the nearest Jellyfish Galaxy IC 3418
DOI: 10.1007/s12036-021-09764-w Bibcode: 2021JApA...42...86H

Hota, Ananda; Devaraj, Ashish; Pradhan, Ananta C. +11 more

We present the far ultraviolet (FUV) imaging of the nearest Jellyfish or Fireball galaxy IC3418/VCC 1217, in the Virgo cluster of galaxies, using Ultraviolet Imaging Telescope (UVIT) onboard the AstroSat satellite. The young star formation observed here in the 17 kpc long turbulent wake of IC3418, due to ram pressure stripping of cold gas surround…

2021 Journal of Astrophysics and Astronomy
eHST 3
Solar EUV-Enhancement and Thermospheric Disturbances
DOI: 10.1029/2021SW002840 Bibcode: 2021SpWea..1902840B

Briand, C.; Doerksen, K.; Deleflie, F.

The increase of energetic electromagnetic flux during solar flares and particle precipitation during geomagnetic activity are among the most important sources of neutral density disturbances to the Earth's thermosphere. However, disentangling the role of X and EUV radiation during solar flares is difficult due to the rarity of sufficiently isolate…

2021 Space Weather
SOHO 3
Mapping Milky Way Halo Substructure Using Stars in the Extended Blue Tail of the Horizontal Branch
DOI: 10.3847/1538-4357/abe385 Bibcode: 2021ApJ...910..102G

Newberg, Heidi Jo; Gryncewicz, Robert; Martin, Charles +2 more

Although blue horizontal branch (BHB) stars are commonly used to trace halo substructure, the stars bluer than (g - r) < -0.3 are ignored owing to the difficulty in determining their absolute magnitudes. The blue extension of the horizontal branch (HBX) includes BHB tail stars and extreme horizontal branch (EHB) stars. We present a method for i…

2021 The Astrophysical Journal
Gaia 3