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Browsing Публикации сотрудников КФУ Scopus by Author "Leto P."

Browsing Публикации сотрудников КФУ Scopus by Author "Leto P."

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  • Leto P.; Trigilio C.; Krtička J.; Fossati L.; Ignace R.; Shultz M.E.; Buemi C.S.; Cerrigone L.; Umana G.; Ingallinera A.; Bordiu C.; Pillitteri I.; Bufano F.; Oskinova L.M.; Agliozzo C.; Cavallaro F.; Riggi S.; Loru S.; Todt H.; Giarrusso M.; Phillips N.M.; Robrade J.; Leone F. (2021)
    In this paper, we present the analysis of incoherent non-thermal radio emission from a sample of hot magnetic stars, ranging from early-B to early-A spectral type. Spanning a wide range of stellar parameters and wind ...
  • Oskinova L.M.; Ignace R.; Leto P.; Postnov K.A. (2020)
    © ESO 2020. Context. KQ Vel is a peculiar A0p star with a strong surface magnetic field of about 7.5 kG. It has a slow rotational period of nearly 8 years. Bailey et al. (A&A, 575, A115) detected a binary companion of ...
  • Leto P.; Trigilio C.; Leone F.; Pillitteri I.; Buemi C.S.; Fossati L.; Cavallaro F.; Oskinova L.M.; Ignace R.; Krtička J.; Umana G.; Catanzaro G.; Ingallinera A.; Bufano F.; Agliozzo C.; Phillips N.M.; Cerrigone L.; Riggi S.; Loru S.; Munari M.; Gangi M.; Giarrusso M.; Robrade J. (2020)
    © 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society We present new ATCA multiwavelength radio measurements (range 2.1–21.2 GHz) of the early-type magnetic star ρ Oph A, ...
  • Carnerero M.; Raiteri C.; Villata M.; Acosta-Pulido J.; D'Ammando F.; Smith P.; Larionov V.; Agudo I.; Arévalo M.; Arkharov A.; Bach U.; Bachev R.; Benítez E.; Blinov D.; Bozhilov V.; Buemi C.; Bueno Bueno A.; Carosati D.; Casadio C.; Chen W.; Damljanovic G.; Di Paola A.; Efimova N.; Ehgamberdiev S.; Giroletti M.; Gómez J.; González-Morales P.; Grinon-Marin A.; Grishina T.; Gurwell M.; Hiriart D.; Hsiao H.; Ibryamov S.; Jorstad S.; Joshi M.; Kopatskaya E.; Kurtanidze O.; Kurtanidze S.; Lähteenmäki A.; Larionova E.; Larionova L.; Lázaro C.; Leto P.; Lin C.; Lin H.; Manilla-Robles A.; Marscher A.; McHardy I.; Metodieva Y.; Mirzaqulov D.; Mokrushina A.; Molina S.; Morozova D.; Nikolashvili M.; Orienti M.; Ovcharov E.; Panwar N.; Pastor Yabar A.; Puerto Giménez I.; Ramakrishnan V.; Richter G.; Rossini M.; Sigua L.; Strigachev A.; Taylor B.; Tornikoski M.; Trigilio C.; Troitskaya Y.; Troitsky I.; Umana G.; Valcheva A.; Velasco S.; Vince O.; Wehrle A.; Wiesemeyer H. (2015)
    © 2015 The Authors. We present an analysis of the multiwavelength behaviour of the blazar OJ 248 at z = 0.939 in the period 2006-2013. We use low-energy data (optical, near-infrared, and radio) obtained by 21 observatories ...
  • Robrade J.; Oskinova L.; Schmitt J.; Leto P.; Trigilio C. (2018)
    © ESO 2018. Context. Among the intermediate-mass magnetic chemically peculiar (MCP) stars, CU Vir is one of the most intriguing objects. Its 100% circularly polarized beams of radio emission sweep the Earth as the star ...
  • Leto P.; Trigilio C.; Buemi C.S.; Leone F.; Pillitteri I.; Fossati L.; Cavallaro F.; Oskinova L.M.; Ignace R.; Krtička J.; Umana G.; Catanzaro G.; Ingallinera A.; Bufano F.; Riggi S.; Cerrigone L.; Loru S.; Schilliró F.; Agliozzo C.; Phillips N.M.; Giarrusso M.; Robrade J. (2020)
    © 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. The non-thermal radio emission of main-sequence early-type stars is a signature of stellar magnetism. We present ...
  • Leto P.; Trigilio C.; M. Oskinova L.; Ignace R.; Buemi C.; Umana G.; Cavallaro F.; Ingallinera A.; Bufano F.; Phillips N.; Agliozzo C.; Cerrigone L.; Todt H.; Riggi S.; Leone F. (2019)
    © 2018 The Author(s). We report the detection of the auroral radio emission from the early-type magnetic star HD142301. New VLA observations of HD142301 detected highly polarized amplified emission occurring at fixed stellar ...
  • Raiteri C.; Villata M.; Smith P.; Larionov V.; Acosta-Pulido J.; Aller M.; D'Ammando F.; Gurwell M.; Jorstad S.; Joshi M.; Kurtanidze O.; Lähteenmäki A.; Mirzaqulov D.; Agudo I.; Aller H.; Arévalo M.; Arkharov A.; Bach U.; Benítez E.; Berdyugin A.; Blinov D.; Blumenthal K.; Buemi C.; Bueno A.; Carleton T.; Carnerero M.; Carosati D.; Casadio C.; Chen W.; Di Paola A.; Dolci M.; Efimova N.; Ehgamberdiev S.; Gómez J.; González A.; Hagen-Thorn V.; Heidt J.; Hiriart D.; Holikov S.; Konstantinova T.; Kopatskaya E.; Koptelova E.; Kurtanidze S.; Larionova E.; Larionova L.; León-Tavares J.; Leto P.; Lin H.; Lindfors E.; Marscher A.; McHardy I.; Molina S.; Morozova D.; Mujica R.; Nikolashvili M.; Nilsson K.; Ovcharov E.; Panwar N.; Pasanen M.; Puerto-Gimenez I.; Reinthal R.; Richter G.; Ros J.; Sakamoto T.; Schwartz R.; Sillanpää A.; Smith N.; Takalo L.; Tammi J.; Taylor B.; Thum C.; Tornikoski M.; Trigilio C.; Troitsky I.; Umana G.; Valcheva A.; Wehrle A. (2012)
    Context. After years of modest optical activity, the quasar-type blazar 4C 38.41 (B3 1633+382) experienced a large outburst in 2011, which was detected throughout the entire electromagnetic spectrum, renewing interest in ...

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