papers

Publications (19)

astro-ph.SR2019

Evolving pulsation of the slowly rotating magnetic Cep star CMa

G. A. Wade, A. Pigulski, S. Begy +11

Recent BRITE-Constellation space photometry of the slowly rotating, magnetic Cep pulsator CMa permits a new analysis of its pulsation properties. Analysis of the two-co…

astro-ph.SR2024

First Observation of the Complete Rotation Period of the Ultra-Slowly Rotating Magnetic O Star HD 54879

C. Erba, C. P. Folsom, A. David-Uraz +6

HD 54879 is the most recently discovered magnetic O-type star. Previous studies ruled out a rotation period shorter than 7 years, implying that HD 54879 is the second most slowly-r…

physics.ed-ph2024

Astronomy in Appalachia: Five Lessons in Designing a Planetarium Show

C. Erba, G. Anderson, T. Cox +2

Cultural Astronomy sits at the intersection of our study of the universe and the human experience, exploring how we observe the stars, interpret their motions, and incorporate them…

astro-ph.SR2019

Magnetic OB[A] Stars with TESS: probing their Evolutionary and Rotational properties -- The MOBSTER Collaboration

A. David-Uraz, C. Neiner, J. Sikora +14

In this contribution, we present the MOBSTER Collaboration, a large community effort to leverage high-precision photometry from the Transiting Exoplanet Survey Satellite (\textit{T…

astro-ph.SR2023

X-Shooting ULLYSES: Massive stars at low metallicity. III. Terminal wind speeds of ULLYSES massive stars

C. Hawcroft, H. Sana, L. Mahy +26

The winds of massive stars have an impact on stellar evolution and on the surrounding medium. The maximum speed reached by these outflows, the terminal wind speed, is a global wind…

astro-ph.SR2022

Ultraviolet Spectropolarimetry With Polstar: Using Polstar to test Magnetospheric Mass-loss Quenching

M. E. Shultz, R. Casini, M. C. M. Cheung +17

Polstar is a proposed NASA MIDEX space telescope that will provide high-resolution, simultaneous full-Stokes spectropolarimetry in the far ultraviolet, together with low-resolution…

astro-ph.SR2021

Ultraviolet Line Profiles of Slowly Rotating Massive Star Winds Using the "Analytic Dynamical Magnetosphere" Formalism

C. Erba, A. David-Uraz, V. Petit +6

Recent large-scale spectropolarimetric surveys have established that a small but significant percentage of massive stars host stable, surface dipolar magnetic fields with strengths…

astro-ph.SR2020

New observations of NGC 1624-2 reveal a complex magnetospheric structure and underlying surface magnetic geometry

A. David-Uraz, V. Petit, M. E. Shultz +5

NGC 1624-2 is the most strongly magnetized O-type star known. Previous spectroscopic observations of this object in the ultraviolet provided evidence that it hosts a large and dens…

astro-ph.SR2018

Extreme resonance line profile variations in the ultraviolet spectra of NGC 1624-2: probing the giant magnetosphere of the most strongly magnetized known O-type star

A. David-Uraz, C. Erba, V. Petit +12

In this paper, we present high-resolution HST/COS observations of the extreme magnetic O star NGC 1624-2. These represent the first ultraviolet spectra of this archetypal object. W…

astro-ph.IM2021

Ultraviolet Spectropolarimetry With Polstar: Hot Star Magnetospheres

M. E. Shultz, R. Casini, M. C. M. Cheung +17

Polstar is a proposed NASA MIDEX space telescope that will provide high-resolution, simultaneous full-Stokes spectropolarimetry in the far ultraviolet, together with low-resolution…

astro-ph.SR2021

MOBSTER -- IV. Detection of a new magnetic B-type star from follow-up spectropolarimetric observations of photometrically selected candidates

A. David-Uraz, M. E. Shultz, V. Petit +8

In this paper, we present results from the spectropolarimetric follow-up of photometrically selected candidate magnetic B stars from the MOBSTER project. Out of four observed targe…

astro-ph.SR2022

Ultraviolet Spectropolarimetry: Investigating stellar magnetic field diagnostics

C. P. Folsom, R. Ignace, C. Erba +9

Magnetic fields are important for stellar photospheres and magnetospheres, influencing photospheric physics and sculpting stellar winds. Observations of stellar magnetic fields are…

astro-ph.SR2019

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.SR2023

Spectroscopic and evolutionary analyses of the binary system AzV 14 outline paths toward the WR stage at low metallicity

D. Pauli, L. M. Oskinova, W. -R. Hamann +16

The origin of the observed population of Wolf-Rayet (WR) stars in low-metallicity (low-Z) galaxies, such as the Small Magellanic Cloud (SMC), is not yet understood. Standard, singl…

astro-ph.SR2018

Massive star winds interacting with magnetic fields on various scales

A. David-Uraz, V. Petit, C. Erba +3

One of the defining processes which govern massive star evolution is their continuous mass loss via dense, supersonic line-driven winds. In the case of those OB stars which also ho…

astro-ph.SR2022

Ultraviolet Spectropolarimetric Diagnostics of Hot Star Magnetospheres

Asif ud-Doula, M. C. M. Cheung, A. David-Uraz +11

Several space missions and instruments for UV spectropolarimetry are in preparation, such as the proposed NASA MIDEX Polstar project, the proposed ESA M mission Arago, and the Poll…

astro-ph.SR2023

X-Shooting ULLYSES: massive stars at low metallicity. I. Project Description

Jorick S. Vink, A. Mehner, P. A. Crowther +78

Observations of individual massive stars, super-luminous supernovae, gamma-ray bursts, and gravitational-wave events involving spectacular black-hole mergers, indicate that the low…

astro-ph.SR2021

Detecting the Zeeman effect in Massive Star Magnetospheres in the UV

C. Erba, V. Petit, K. Gayley +3

Approximately 7% of massive stars host stable surface magnetic fields that are strong enough to alter stellar evolution through their effect on the stellar wind. It is therefore cr…

astro-ph.SR2021

Confirmation of xi^1 CMa's ultra-slow rotation: magnetic polarity reversal and a dramatic change in magnetospheric UV emission lines

C. Erba, M. E. Shultz, V. Petit +5

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 t…