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Numrering	Referens	Omslagsbild	Hitta
1.	Erba, C., et al. (författare) Confirmation of ξ1 CMa’s ultra-slow rotation : magnetic polarity reversal and a dramatic change in magnetospheric UV emission lines 2021 Ingår i: Monthly notices of the Royal Astronomical Society. - : Oxford University Press. - 0035-8711 .- 1365-2966. ; 506:2, s. 2296-2308 Tidskriftsartikel (refereegranskat)abstract The magnetic beta Cep pulsator xi(1) CMa has the longest rotational period of any known magnetic B-type star. It is also the only magnetic B-type star with magnetospheric emission that is known to be modulated by both rotation and pulsation. We report here the first unambiguous detection of a negative longitudinal magnetic field in xi(1) CMa (< B-z > = -87 +/- 2 G in 2019 and < B-z > = -207 +/- 3 G in 2020), as well as the results of ongoing monitoring of the star's H alpha variability. We examine evidence for deviation from a purely dipolar topology. We also report a new HST UV spectrum of xi(1) CMa obtained near magnetic null that is consistent with an equatorial view of the magnetosphere, as evidenced by its similarity to the UV spectrum of beta Cep obtained near maximum emission. The new UV spectrum of xi(1) CMa provides additional evidence for the extremely long rotation period of this star via comparison to archival data.

Erba, C., et al. (författare)
Confirmation of ξ1 CMa’s ultra-slow rotation : magnetic polarity reversal and a dramatic change in magnetospheric UV emission lines
2021
Ingår i: Monthly notices of the Royal Astronomical Society. - : Oxford University Press. - 0035-8711 .- 1365-2966. ; 506:2, s. 2296-2308
Tidskriftsartikel (refereegranskat)abstract
- The magnetic beta Cep pulsator xi(1) CMa has the longest rotational period of any known magnetic B-type star. It is also the only magnetic B-type star with magnetospheric emission that is known to be modulated by both rotation and pulsation. We report here the first unambiguous detection of a negative longitudinal magnetic field in xi(1) CMa (< B-z > = -87 +/- 2 G in 2019 and < B-z > = -207 +/- 3 G in 2020), as well as the results of ongoing monitoring of the star's H alpha variability. We examine evidence for deviation from a purely dipolar topology. We also report a new HST UV spectrum of xi(1) CMa obtained near magnetic null that is consistent with an equatorial view of the magnetosphere, as evidenced by its similarity to the UV spectrum of beta Cep obtained near maximum emission. The new UV spectrum of xi(1) CMa provides additional evidence for the extremely long rotation period of this star via comparison to archival data.

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