Search Results - "Prišegen, M"

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    Magnetic chemically peculiar stars investigated by the Solar Mass Ejection Imager by Paunzen, E, Supíková, J, Bernhard, K, Hümmerich, S, Prišegen, M

    “…ABSTRACT Since the discovery of the spectral peculiarities of their prototype α2 Canum Venaticorum in 1897, the so-called ACV variables, which are comprised of…”
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    Journal Article
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    Uncovering new white dwarf - open cluster associations using Gaia DR3 by Prišegen, M, Faltová, N

    Published 03-07-2023
    “…A&A 678, A20 (2023) Context: Open clusters (OCs) provide homogeneous samples of white dwarfs (WDs) with known distances, extinctions, and total ages. The…”
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    Kinematic distinction of the two subpopulations of X-ray pulsars by Prišegen, M

    Published 09-07-2020
    “…A&A 640, A86 (2020) The population of Be/X-ray binaries shows strong evidence of bimodality, especially in the spin period of neutron stars. Several physical…”
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    New ACV variables discovered in the Zwicky Transient Facility survey by Bauer-Fasching, B, Bernhard, K, Brändli, E, Burger, H, Eisele, B, Hümmerich, S, Neuhold, J, Paunzen, E, Piecka, M, Ratzenböck, S, Prišegen, M

    Published 10-06-2024
    “…The manifestation of surface spots on magnetic chemically peculiar (mCP) stars is most commonly explained by the atomic diffusion theory, which requires a calm…”
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    White dwarf-open cluster associations based on Gaia DR2 by Prišegen, M, Piecka, M, Faltová, N, Kajan, M, Paunzen, E

    Published 06-11-2020
    “…A&A 645, A13 (2021) Fundamental parameters and physical processes leading to the formation of white dwarfs (WDs) may be constrained and refined by discovering…”
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    Chemically peculiar stars on the pre-main sequence by Kueß, L, Paunzen, E, Faltová, N, Jadlovský, D, Labaj, M, Mesarč, M, Mondal, P, Prišegen, M, Ramezani, T, Supíková, J, Svačinková, K, Vítková, M, Xia, C, Bernhard, K, Hümmerich, S

    Published 14-05-2024
    “…A&A 687, A176 (2024) Context. The chemically peculiar (CP) stars of the upper main sequence are defined by spectral peculiarities that indicate unusual…”
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    A case study of ACV variables discovered in the Zwicky Transient Facility survey by Faltová, N, Kallová, K, Prišegen, M, Staněk, P, Supíková, J, Xia, C, Bernhard, K, Hümmerich, S, Paunzen, E

    Published 25-08-2021
    “…A&A 656, A125 (2021) Magnetic chemically peculiar (mCP) stars exhibit complex atmospheres that allow the investigation of the interplay of atomic diffusion,…”
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    The detection of magnetic chemically peculiar stars using Gaia BP/RP spectra by Paunzen, E, Prisegen, M

    Published 05-10-2022
    “…A&A 667, L10 (2022) The magnetic chemically peculiar (mCP) stars of the upper main sequence are perfectly suited to studying the effects of rotation,…”
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    Concerning the occurrence of bow shocks around high-mass X-ray binaries by Prisegen, M

    Published 16-11-2018
    “…A&A 621, A37 (2019) We investigate the occurrence of stellar bow shocks around high-mass X-ray binaries (HMXBs) in the Galaxy. We seek to conduct a survey of…”
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    An all-sky catalogue of stellar reddening values by Paunzen, E, Netopil, M, Prisegen, M, Faltova, N

    Published 31-07-2024
    “…When observing astronomical objects, we must deal with extinction (i.e. the absorption and scattering of the emitted radiation by dust and gas between the…”
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  16. 16

    Magnetic chemically peculiar stars investigated by the Solar Mass Ejection Imager by Paunzen, E, Supikova, J, Bernhard, K, Huemmerich, S, Prisegen, M

    Published 05-05-2021
    “…Since the discovery of the spectral peculiarities of their prototype alpha2 Canum Venaticorum in 1897, the so-called ACV variables, which are comprised of…”
    Get full text
    Journal Article
  17. 17

    Rotational modulation and single g-mode pulsation in the B9pSi star HD174356? by Mikulasek, Z, Paunzen, E, Huemmerich, S, Niemczura, E, Walczak, P, Fraga, L, Bernhard, K, Janik, J, Hubrig, S, Jaervinen, S, Jagelka, M, Pintado, O. I, Krticka, J, Prisegen, M, Skarka, M, Zejda, M, Ilyin, I, Pribulla, T, Kaminski, K, Kaminska, M. K, Tokarek, J, Zielinski, P

    Published 06-08-2020
    “…Chemically peculiar (CP) stars of the upper main sequence are characterised by specific anomalies in the photospheric abundances of some chemical elements. The…”
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