activity
20152019
most citedThe Magnetic Early B-type Stars I: Magnetometry and Rotation

101 citations · 337 across the 11 of their papers we have counts for

collaborators

12 papers

astro-ph.SR201922 cited

Lupi: measuring the heartbeat of a doubly-magnetic massive binary with BRITE-Constellation

H. Pablo, M. Shultz, J. Fuller +15

Lupi A is a binary system consisting of two main sequence early B-type stars Aa and Ab in a short period, moderately eccentric orbit. The close binary pair is the onl…

astro-ph.SR201923 cited

The accelerating rotation of the magnetic He-weak star HD 142990

M. Shultz, Th. Rivinius, B. Das +2

HD 142990 (V 913 Sco; B5 V) is a He-weak star with a strong surface magnetic field and a short rotation period ( d). While it is clearly a rapid rotator, recent…

astro-ph.SR201958 cited

Magnetic OB[A] Stars with TESS: probing their Evolutionary and Rotational properties (MOBSTER) - I. First-light observations of known magnetic B and A stars

A. David-Uraz, C. Neiner, J. Sikora +21

In this paper we introduce the MOBSTER collaboration and lay out its scientific goals. We present first results based on the analysis of nineteen previously known magnetic O, B and…

astro-ph.SR201922 cited

Detection of coherent emission from the Bp star HD 142990 at uGMRT frequencies

Barnali Das, Poonam Chandra, M. E. Shultz +1

HD 142990 is a Bp-type star with a nearly dipolar surface magnetic field of kG strength. Recently Lenc et al. (2018) reported the tentative discovery of Electron Cyclotron Maser Em…

astro-ph.SR2018101 cited

The Magnetic Early B-type Stars I: Magnetometry and Rotation

M. E. Shultz, G. A. Wade, Th. Rivinius +7

The rotational and magnetic properties of many magnetic hot stars are poorly characterized, therefore the MiMeS and BinaMIcS collaborations have collected extensive high-dispersion…

astro-ph.SR201734 cited

HD 156324: a tidally locked magnetic triple spectroscopic binary with a disrupted magnetosphere

M. Shultz, Th. Rivinius, G. A. Wade +3

HD 156324 is an SB3 (B2V/B5V/B5V) system in the Sco OB4 association. The He-strong primary possesses both a strong magnetic field, and H emission believed to originate in its Ce…