activity
20072026
most citedSurface magnetism of cool stars

32 citations · 80 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.SR2026

Magnetic field, rotation, and binarity of the first magnetic B[e] star, IRAS 17449+2320

I. Bermejo Lozano, G. A. Wade, C. P. Folsom +1

IRAS 17449+2320 is the first identified magnetic B[e] star. It belongs to a subgroup of peculiar hot B-type stars, called FS~CMa stars. presenting the B[e] phenomenon, i.e., permit…

astro-ph.SR2026★ 3 cited

Intermediate-Mass Mergers: A New Scenario for Several FS CMa Stars

Daniela Korcakova, Nela Dvorakova, Iris Bermejo Lozano +6

We summarise the properties and nature of a peculiar group of B-type stars called FS CMa stars. These stars show the B[e] phenomenon, i.e., their spectra exhibit both forbidden emi…

astro-ph.SR2026

The rotational and magnetic properties of Polaris from long-term spectropolarimetric monitoring

James A. Barron, Gregg A. Wade, Colin P. Folsom

Polaris is a highly unusual Cepheid with observed properties that are difficult to reconcile with stellar evolutionary models. Since the initial detection of Polaris' magnetic fiel…

astro-ph.IM2025★ 12 cited

SpecpolFlow: a new software package for spectropolarimetry using Python

Colin P. Folsom, Christiana Erba, Veronique Petit +8

Spectropolarimetry, the observation of polarization and intensity as a function of wavelength, is a powerful tool in stellar astrophysics. It is particularly useful for characteriz…

astro-ph.SR2019★ 5 cited

No evidence of a sudden change of spectral appearance or magnetic field strength of the O9.7V star HD 54879

G. A. Wade, S. Bagnulo, Z. Keszthelyi +8

It was recently claimed that the magnetic O-type star HD 54879 exhibits important radial velocity variability indicative of its presence in a spectroscopic binary. More remarkably,…

astro-ph.SR2016★ 32 cited

Surface magnetism of cool stars

O. Kochukhov, P. Petit, K. G. Strassmeier +10

Magnetic fields are essential ingredients of many physical processes in the interiors and envelopes of cool stars. Yet their direct detection and characterisation is notoriously di…

astro-ph.SR2013★ 1 cited

Chemical peculiarities in magnetic and non-magnetic pre-main sequence A and B stars

C. P. Folsom, S. Bagnulo, G. A. Wade +2

In A- and late B-type stars, strong magnetic fields are always associated with Ap and Bp chemical peculiarities. However, it is not clear at what point in a star's evolution those…

astro-ph.SR2010★ 24 cited

A detailed spectroscopic analysis of the open cluster NGC 5460

L. Fossati, C. P. Folsom, S. Bagnulo +5

Within the context of a large project aimed at studying early F-, A- and late B-type stars we present the abundance analysis of the photospheres of 21 members of the open cluster N…

astro-ph2007

How non-magnetic are "non-magnetic" Herbig Ae/Be stars?

G. A. Wade, E. Alecian, C. Catala +9

Our recent discovery of magnetic fields in a small number of Herbig Ae/Be stars has required that we survey a much larger sample of stars. From our FORS1 and ESPaDOnS surveys, we h…

astro-ph2007★ 3 cited

Magnetic, Chemical and Rotational Properties of the Herbig Ae/Be Binary System HD 72106

C. P. Folsom, G. A. Wade, O. Kochukhov +5

Recently, strong, globally-ordered magnetic fields have been detected in some Herbig Ae and Be (HAeBe) stars, suggesting a possible evolutionary connection to main sequence magneti…