activity
20152025
most citedBRITE-Constellation high-precision time-dependent photometry of the early-O-type supergiant Puppis unveils the photospheric drivers of its small- and large-scale wind structures

70 citations · 409 across the 29 of their papers we have counts for

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Showing 2020Show all

8 papers · 1 filter

astro-ph.SR20207 cited

New BRITE-Constellation observations of the roAp star Alpha Circini

W. W. Weiss, H. -E. Fröhlich, T. Kallinger +11

Chemically peculiar (CP) stars with a measurable magnetic field comprise the group of mCP stars. The pulsating members define the subgroup of rapidly oscillating Ap (roAp) stars, o…

astro-ph.IM2020

Point Spread Function Estimation for Wide Field Small Aperture Telescopes with Deep Neural Networks and Calibration Data

Peng Jia, Xuebo Wu, Zhengyang Li +4

The point spread function (PSF) reflects states of a telescope and plays an important role in development of data processing methods, such as PSF based astrometry, photometry and i…

astro-ph.SR2020

BRITE photometry and STELLA spectroscopy of bright stars in Auriga: Rotation, pulsation, orbits, and eclipses

K. G. Strassmeier, T. Granzer, M. Weber +7

Continuous photometry with up to three BRITE satellites was obtained for 12 targets and subjected to a period search. Contemporaneous high-resolution optical spectroscopy with STEL…

astro-ph.SR2020

beta Cas: the first delta Scuti star with a dynamo magnetic field

K. Zwintz, C. Neiner, O. Kochukhov +10

F type stars are characterised by several physical processes such as different pulsation mechanisms, rotation, convection, diffusion, and magnetic fields. The rapidly rotating delt…

astro-ph.SR202013 cited

BRITE-Constellation photometry of $\bpi^5$ Orionis, an ellipsoidal SPB variable

M. Jerzykiewicz, A. Pigulski, G. Handler +5

Results of an analysis of the BRITE-Constellation photometry of the SB1 system and ellipsoidal variable Ori (B2\,III) are presented. In addition to the orbital light-variatio…

astro-ph.HE2020

Direct evidence for shock-powered optical emission in a nova

Elias Aydi, Kirill V. Sokolovsky, Laura Chomiuk +39

Classical novae are thermonuclear explosions that occur on the surfaces of white dwarf stars in interacting binary systems (Bode & Evans 2008). It has long been thought that the lu…