217 citations · 1.9k across the 83 of their papers we have counts for
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HI 21 cm observation and mass models of the extremely thin galaxy FGC 1440
K. Aditya, Peter Kamphuis, Arunima Banerjee +4
We present observations and models of the kinematics and distribution of neutral hydrogen (HI) in the superthin galaxy FGC 1440 with an optical axial ratio . Using the…
Fractal dimension of optical cirrus in Stripe82
Alexander A. Marchuk, Anton A. Smirnov, Aleksandr V. Mosenkov +4
The geometric characteristics of dust clouds provide important information on the physical processes that structure such clouds. One of such characteristics is the fractal dim…
Isochrone fitting of Galactic globular clusters -- III. NGC\,288, NGC\,362, and NGC\,6218 (M12)
George A. Gontcharov, Maxim Yu. Khovritchev, Aleksandr V. Mosenkov +6
We present new isochrone fits to colour-magnitude diagrams of the Galactic globular clusters NGC\,288, NGC\,362, and NGC\,6218 (M12). We utilize a lot of photometric bands from the…
The structure of the Milky Way based on unWISE 3.4m integrated photometry
Aleksandr V. Mosenkov, Sergey S. Savchenko, Anton A. Smirnov +1
We present a detailed analysis of the Galaxy structure using an unWISE wide-field image at m. We perform a 3D photometric decomposition of the Milky Way taking into account i…
Probing the spectral shape of dust emission with the DustPedia galaxy sample
Angelos Nersesian, Wouter Dobbels, Manolis E. Xilouris +10
The objective of this paper is to understand the variance of the far-infrared (FIR) spectral energy distribution (SED) of the DustPedia galaxies, and its link with the stellar and…
Quantified diffuse light in compact groups of galaxies
Denis Poliakov, Aleksandr V. Mosenkov, Noah Brosch +2
The vast majority of stars in galaxy groups are contained within their constituent galaxies. Some small fraction of stars is expected, however, to follow the global dark matter pot…