Search Results - "Shultz, E"
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1
The magnetic early B-type stars I: magnetometry and rotation
Published in Monthly notices of the Royal Astronomical Society (2018)“…Abstract The rotational and magnetic properties of many magnetic hot stars are poorly characterized, therefore the Magnetism in Massive Stars and Binarity and…”
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2
XMM-Newton Perspective of the Unique Magnetic Binary-ϵ Lupi
Published in The Astrophysical journal (01-10-2024)“…Abstract The ϵ Lupi A (HD 136504) system stands out among magnetic massive binaries as the only short-period binary system in which both components have…”
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3
Operational Implementation of Prospective Genotyping for Personalized Medicine: The Design of the Vanderbilt PREDICT Project
Published in Clinical pharmacology and therapeutics (01-07-2012)“…The promise of “personalized medicine” guided by an understanding of each individual's genome has been fostered by increasingly powerful and economical methods…”
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4
Unstable Phenomena in Stable Magnetospheres: Searching for Radio Flares from Magnetic OBA Stars Using VCSS
Published in The Astrophysical journal (01-12-2023)“…Abstract Although the majority of hot magnetic stars have extremely stable, ∼kilogauss strength surface magnetic fields with simple topologies, a subset…”
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5
Fertility-related knowledge and reproductive goals in childhood cancer survivors: short communication
Published in Human reproduction (Oxford) (01-11-2017)“…Abstract STUDY QUESTION Do young adult survivors of childhood cancer know their fertility status, in the context of their parenthood goals and screening for…”
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Exploring nine simultaneously occurring transients on April 12th 1950
Published in Scientific reports (17-06-2021)“…Nine point sources appeared within half an hour on a region within ∼ 10 arcmin of a red-sensitive photographic plate taken in April 1950 as part of the…”
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APPLICATION OF THE METHOD OF DIFFERENTIAL CONSTRAINTS TO SYSTEMS OF EQUATIONS WRITTEN IN RIEMANN INVARIANTS
Published in Journal of applied mechanics and technical physics (01-05-2021)“…Solutions of one-dimensional equations of gas dynamics and the equations describing the behavior of a nonlinear elastic material are reduced to solving a…”
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8
Detection of Coherent Emission from the Bp Star HD 142990 at uGMRT Frequencies
Published in The Astrophysical journal (01-06-2019)“…HD 142990 is a Bp-type star with a nearly dipolar surface magnetic field of kilogauss strength. Recently, Lenc et al. reported the tentative discovery of…”
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The fifth main-sequence magnetic B-type star showing coherent radio emission: Is this really a rare phenomenon?
Published in Monthly notices of the Royal Astronomical Society. Letters (01-10-2019)“…ABSTRACT We report the discovery of intense, highly directional radio emission from the Bp star HD 35298, which we interpret as the consequence of Electron…”
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10
Using ZDI maps to determine magnetic forces and torques at the photospheres of early-type stars
Published in Monthly notices of the Royal Astronomical Society (25-04-2024)“…ABSTRACT We use the magnetic field components measured by Zeeman Doppler imaging (ZDI) to calculate the stellar surface force and torque due to magnetic…”
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11
Comparison of screening methods for antibiotics in beef kidney juice and serum
Published in Analytica chimica acta (01-04-2009)“…Rapid screening tests can be used as part of an efficient program designed to monitor veterinary drug residues in cattle. In this work, three rapid tests…”
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Journal Article Conference Proceeding -
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The magnetic early B-type stars – III. A main-sequence magnetic, rotational, and magnetospheric biography
Published in Monthly notices of the Royal Astronomical Society (21-11-2019)“…ABSTRACT Magnetic confinement of stellar winds leads to the formation of magnetospheres, which can be sculpted into centrifugal magnetospheres (CMs) by…”
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How the breakout-limited mass in B-star centrifugal magnetospheres controls their circumstellar H α emission
Published in Monthly notices of the Royal Astronomical Society (01-12-2020)“…ABSTRACT Strongly magnetic B-type stars with moderately rapid rotation form ‘centrifugal magnetospheres’ (CMs) from the magnetic trapping of stellar wind…”
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Centrifugal breakout reconnection as the electron acceleration mechanism powering the radio magnetospheres of early-type stars
Published in Monthly notices of the Royal Astronomical Society (29-04-2022)“…ABSTRACT Magnetic B-stars often exhibit circularly polarized radio emission thought to arise from gyrosynchrotron emission by energetic electrons trapped in…”
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The effects of surface fossil magnetic fields on massive star evolution – II. Implementation of magnetic braking in mesa and implications for the evolution of surface rotation in OB stars
Published in Monthly notices of the Royal Astronomical Society (01-03-2020)“…ABSTRACT The time evolution of angular momentum and surface rotation of massive stars are strongly influenced by fossil magnetic fields via magnetic braking…”
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Testing a scaling relation between coherent radio emission and physical parameters of hot magnetic stars
Published in Monthly notices of the Royal Astronomical Society (10-11-2022)“…ABSTRACT Coherent radio emission via electron cyclotron maser emission (ECME) from hot magnetic stars was discovered more than two decades ago, but the…”
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Discovery of Eight “Main-sequence Radio Pulse Emitters” Using the GMRT: Clues to the Onset of Coherent Radio Emission in Hot Magnetic Stars
Published in The Astrophysical journal (01-02-2022)“…Abstract Main-sequence radio pulse emitters (MRPs) are magnetic early-type stars from which periodic radio pulses, produced via electron cyclotron maser…”
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The magnetic early B-type stars – IV. Breakout or leakage? H α emission as a diagnostic of plasma transport in centrifugal magnetospheres
Published in Monthly notices of the Royal Astronomical Society (01-12-2020)“…ABSTRACT Rapidly rotating early-type stars with strong magnetic fields frequently show H α emission originating in centrifugal magnetospheres (CMs),…”
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Electron scattering emission in the light curves of stars with centrifugal magnetospheres
Published in Monthly notices of the Royal Astronomical Society (02-03-2022)“…ABSTRACT Strongly magnetic, rapidly rotating B-type stars with relatively weak winds form centrifugal magnetospheres (CMs), as the stellar wind becomes…”
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MOBSTER – VI. The crucial influence of rotation on the radio magnetospheres of hot stars
Published in Monthly notices of the Royal Astronomical Society (29-04-2022)“…ABSTRACT Numerous magnetic hot stars exhibit gyrosynchrotron radio emission. The source electrons were previously thought to be accelerated to relativistic…”
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