papers

Publications (24)

astro-ph.SR2017

The metallicity dependence of WR winds

R. Hainich, T. Shenar, A. Sander +2

Wolf-Rayet (WR) stars are the most advanced stage in the evolution of the most massive stars. The strong feedback provided by these objects and their subsequent supernova (SN) expl…

cond-mat.supr-con2017

A high-temperature superconducting weak-link defined by ferroelectric field-effect

L. Begon-Lours, V. Rouco, A. Sander +10

In all-oxide ferroelectric (FE) - superconductor (S) bilayers, due to the low carrier concentration of oxides compared to transition metals, the FE interfacial polarization charges…

cond-mat.supr-con2020

Long-Range Propagation and Interference of -wave Superconducting Pairs in Graphene

D. Perconte, K. Seurre, V. Humbert +13

Recent experiments have shown that proximity with high-temperature superconductors induces unconventional superconducting correlations in graphene. Here we demonstrate that those c…

astro-ph.SR2014

Discovery of a new Wolf-Rayet star and a candidate star cluster in the Large Magellanic Cloud with Spitzer

V. V. Gvaramadze, A. -N. Chene, A. Y. Kniazev +8

We report the first-ever discovery of a Wolf-Rayet (WR) star in the Large Magellanic Cloud via detection of a circular shell with the Spitzer Space Telescope. Follow-up observation…

cond-mat.mtrl-sci2021

Spin pumping in d-wave superconductor/ferromagnet hybrids

S. J. Carreira, D. Sanchez-Manzano, M. -W. Yoo +5

Spin-pumping across ferromagnet/superconductor (F/S) interfaces has attracted much attention lately. Yet the focus has been mainly on s-wave superconductors-based systems whereas (…

astro-ph.SR2013

One of the most massive stars in the Galaxy may have formed in isolation

L. M. Oskinova, M. Steinke, W. -R. Hamann +3

Very massive stars, 100 times heavier than the sun, are rare. It is not yet known whether such stars can form in isolation or only in star clusters. The answer to this question is…

cond-mat.mtrl-sci2023

Size-dependence and high temperature stability of radial vortex magnetic textures imprinted by superconductor stray fields

D. Sanchez-Manzano, G. Orfila, A. Sander +15

Swirling spin textures, including topologically non-trivial states, such as skyrmions, chiral domain walls, and magnetic vortices, have garnered significant attention within the sc…

astro-ph.HE2010

The Discovery of gamma-Ray Emission From The Blazar RGB J0710+591

V. A. Acciari, E. Aliu, T. Arlen +234

The high-frequency-peaked BL Lacertae object RGB J0710+591 was observed in the very high-energy (VHE; E > 100 GeV) wave band by the VERITAS array of atmospheric Cherenkov telescope…

astro-ph.CO2010

Observations of Milky Way Dwarf Spheroidal galaxies with the Fermi-LAT detector and constraints on Dark Matter models

LAT Collaboration, A. A. Abdo, M. Ackermann +160

We report on the observations of 14 dwarf spheroidal galaxies with the Fermi Gamma-Ray Space Telescope taken during the first 11 months of survey mode operations. The Fermi telesco…

astro-ph.SR2016

Wolf-Rayet stars in the Small Magellanic Cloud: II. Analysis of the binaries

T. Shenar, R. Hainich, H. Todt +7

Massive WR stars are evolved massive stars characterized by strong mass-loss. Hypothetically, they can form either as single stars or as mass donors in close binaries. About 40% of…

cond-mat.mtrl-sci2019

Factors limiting ferroelectric field-effect doping in complex-oxide heterostructures

L. Bégon-Lours, V. Rouco, Qiao Qiao +12

Ferroelectric field-effect doping has emerged as a powerful approach to manipulate the ground state of correlated oxides, opening the door to a new class of field-effect devices. H…

astro-ph.SR2016

The Tarantula Massive Binary Monitoring project: II. A first SB2 orbital and spectroscopic analysis for the Wolf-Rayet binary R145

T. Shenar, N. D. Richardson, D. P. Sablowski +19

We present the first SB2 orbital solution and disentanglement of the massive Wolf-Rayet binary R145 (P = 159d) located in the Large Magellanic Cloud. The primary was claimed to hav…

astro-ph.GA2010

Radio and Gamma-Ray Constraints on the Emission Geometry and Birthplace of PSR J2043+2740

A. Noutsos, A. A. Abdo, M. Ackermann +146

We report on the first year of Fermi gamma-ray observations of pulsed high-energy emission from the old PSR J2043+2740. The study of the gamma-ray efficiency of such old pulsars gi…

astro-ph.CO2010

Constraints on Cosmological Dark Matter Annihilation from the Fermi-LAT Isotropic Diffuse Gamma-Ray Measurement

LAT collaboration, A. A. Abdo, M. Ackermann +147

The first published Fermi large area telescope (Fermi-LAT) measurement of the isotropic diffuse gamma-ray emission is in good agreement with a single power law, and is not showing…

astro-ph.SR2014

The rapid evolution of the exciting star of the Stingray Nebula

N. Reindl, T. Rauch, M. Parthasarathy +5

SAO244567, the exciting star of the Stingray nebula, is rapidly evolving. Previous analyses suggested that it has heated up from an effective temperature of about 21kK in 1971 to o…

astro-ph.HE2016

Measuring the stellar wind parameters in IGR J17544-2619 and Vela X-1 constrains the accretion physics in Supergiant Fast X-ray Transient and classical Supergiant X-ray Binaries

A. Gimenez-Garcia, T. Shenar, J. M. Torrejon +9

Classical Supergiant X-ray Binaries (SGXBs) and Supergiant Fast X-ray Transients (SFXTs) are two types of High-mass X-ray Binaries (HMXBs) that present similar donors but, at the s…

astro-ph.SR2016

Analysis of the WN star WR 102c, its WR nebula, and the associated cluster of massive stars in the Sickle Nebula

M. Steinke, L. M. Oskinova, W. -R. Hamann +3

The massive Wolf-Rayet type star WR 102c is located near the Quintuplet Cluster - one of the three massive star clusters in the Galactic Center region. Previous studies indicated t…

physics.ins-det2018

Study of radon reduction in gases for rare event search experiments

K. Pushkin, C. Akerlof, D. Anbajagane +15

The noble elements, argon and xenon, are frequently employed as the target and event detector for weakly interacting particles such as neutrinos and Dark Matter. For such rare proc…

astro-ph.SR2013

Very Massive Stars (VMS) in the Local Universe

Jorick S. Vink, Alexander Heger, Mark R. Krumholz +25

Recent studies have claimed the existence of very massive stars (VMS) up to 300 solar masses in the local Universe. As this finding may represent a paradigm shift for the canonical…

astro-ph.HE2010

Fermi LAT Search for Photon Lines from 30 to 200 GeV and Dark Matter Implications

The Fermi LAT Collaboration, A. A. Abdo, M. Ackermann +160

Dark matter (DM) particle annihilation or decay can produce monochromatic -rays readily distinguishable from astrophysical sources. -ray line limits from 30 GeV to 200 GeV…

astro-ph.HE2011

Simultaneous multi-wavelength campaign on PKS 2005-489 in a high state

The H. E. S. S. Collaboration, the Fermi LAT Collaboration, : +345

The high-frequency peaked BL Lac object PKS 2005-489 was the target of a multi-wavelength campaign with simultaneous observations in the TeV gamma-ray (H.E.S.S.), GeV gamma-ray (Fe…

astro-ph.HE2024

Not just winds: why models find binary black hole formation is metallicity dependent, while binary neutron star formation is not

L. A. C. van Son, S. K. Roy, I. Mandel +6

Both detailed and rapid population studies alike predict that binary black hole (BHBH) formation is orders of magnitude more efficient at low metallicity than high metallicity, whi…

astro-ph.SR2015

Wolf-Rayet stars in the Small Magellanic Cloud: I. Analysis of the single WN stars

R. Hainich, D. Pasemann, H. Todt +3

Wolf-Rayet (WR) stars have a severe impact on their environments owing to their strong ionizing radiation fields and powerful stellar winds. Since these winds are considered to be…

cond-mat.supr-con2020

Tailored flux pinning in superconductor/ferromagnet multilayers with engineered magnetic domain morphology from stripes to skyrmions

X. Palermo, N. Reyren, S. Mesoraca +9

Superconductor/Ferromagnet (S/F) hybrid systems show interesting magneto-transport behaviors that result from the transfer of properties between both constituents. For instance, ma…