Search Results - "SCHNEIDER, N. R"
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Binary Interaction Dominates the Evolution of Massive Stars
Published in Science (American Association for the Advancement of Science) (27-07-2012)“…The presence of a nearby companion alters the evolution of massive stars in binary systems, leading to phenomena such as stellar mergers, x-ray binaries, and…”
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3D simulations of strongly magnetized non-rotating supernovae: explosion dynamics and remnant properties
Published in Monthly notices of the Royal Astronomical Society (01-01-2023)“…ABSTRACT We investigate the impact of strong initial magnetic fields in core-collapse supernovae of non-rotating progenitors by simulating the collapse and…”
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THE INCIDENCE OF STELLAR MERGERS AND MASS GAINERS AMONG MASSIVE STARS
Published in The Astrophysical journal (10-02-2014)“…Because the majority of massive stars are born as members of close binary systems, populations of massive main-sequence stars contain stellar mergers and…”
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An excess of massive stars in the local 30 Doradus starburst
Published in Science (American Association for the Advancement of Science) (05-01-2018)“…The 30 Doradus star-forming region in the Large Magellanic Cloud is a nearby analog of large star-formation events in the distant universe. We determined the…”
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Bimodal Black Hole Mass Distribution and Chirp Masses of Binary Black Hole Mergers
Published in Astrophysical journal. Letters (01-06-2023)“…Abstract In binary black hole mergers from isolated binary-star evolution, both black holes are from progenitor stars that have lost their hydrogen-rich…”
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Hydrodynamical simulations and similarity relations for eruptive mass-loss from massive stars
Published in Monthly notices of the Royal Astronomical Society (01-05-2019)Get full text
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Stellar mergers as the origin of magnetic massive stars
Published in Nature (London) (01-10-2019)“…About ten per cent of ‘massive’ stars (those of more than 1.5 solar masses) have strong, large-scale surface magnetic fields 1 – 3 . It has been suggested that…”
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Characterization of a breast cancer cell line derived from a germ-line BRCA1 mutation carrier
Published in Cancer research (Chicago, Ill.) (01-08-1998)“…A tumor cell line, HCC1937, was established from a primary breast carcinoma from a 24-year-old patient with a germ-line BRCA1 mutation. A corresponding…”
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Mutations of the hSNF5/INI1 Gene in Renal Rhabdoid Tumors With Second Primary Brain Tumors
Published in JNCI : Journal of the National Cancer Institute (19-04-2000)“…About 10%-15% of rhabdoid tumors of the kidney in young infants are associated with separate primary tumors of the central nervous system. Demographic and…”
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All patients with the T(11;16)(q23;p13.3) that involves MLL and CBP have treatment-related hematologic disorders
Published in Blood (15-07-1997)“…The involvement of 11q23-balanced translocations in acute leukemia after treatment with drugs that inhibit the function of DNA topoisomerase II (topo II) is…”
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Secondary acute myeloid leukemia in children with acute lymphoblastic leukemia treated with etoposide
Published in Journal of clinical oncology (01-02-1993)“…To describe the occurrence of secondary acute myeloid leukemia (AML) in children with acute lymphoblastic leukemia (ALL) treated with etoposide (VP-16). Two…”
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Simulating the formation of η Carinae’s surrounding nebula through unstable triple evolution and stellar merger-induced eruption
Published in Monthly notices of the Royal Astronomical Society (01-05-2021)“…ABSTRACT η Carinae is an extraordinary massive star famous for its 19th century Great Eruption and the surrounding Homunculus nebula ejected in that event. The…”
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New recurring cytogenetic abnormalities and association of blast cell karyotypes with prognosis in childhood T-cell acute lymphoblastic leukemia: a Pediatric Oncology Group report of 343 cases
Published in Blood (01-10-2000)“…To further define the cytogenetic differences between B-cell lineage (B-lineage) acute lymphoblastic leukemia (ALL) and T-cell lineage ALL (T-ALL) and to…”
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Long-term evolution of a magnetic massive merger product
Published in Monthly notices of the Royal Astronomical Society (01-07-2020)“…ABSTRACT About 10 per cent of stars more massive than ${\approx}1.5\, {\mathrm{M}}_{\odot }$ have strong, large-scale surface magnetic fields and are being…”
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EVOLUTION OF MASS FUNCTIONS OF COEVAL STARS THROUGH WIND-MASS LOSS AND BINARY INTERACTIONS
Published in The Astrophysical journal (20-05-2015)“…ABSTRACT Accurate determinations of stellar mass functions and ages of stellar populations are crucial to much of astrophysics. We analyze the evolution of…”
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The R136 star cluster dissected with Hubble Space Telescope/STIS – II. Physical properties of the most massive stars in R136
Published in Monthly notices of the Royal Astronomical Society (01-12-2020)“…ABSTRACT We present an optical analysis of 55 members of R136, the central cluster in the Tarantula Nebula of the Large Magellanic Cloud. Our sample was…”
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Primary body cavity-based AIDS-related lymphomas
Published in American journal of clinical pathology (01-02-1996)“…Five patients with advanced AIDS developed a unique type of high grade primary body cavity-based non-Hodgkin's lymphoma (NHL). The lymphomas were exclusively…”
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AGES OF YOUNG STAR CLUSTERS, MASSIVE BLUE STRAGGLERS, AND THE UPPER MASS LIMIT OF STARS: ANALYZING AGE-DEPENDENT STELLAR MASS FUNCTIONS
Published in The Astrophysical journal (10-01-2014)“…Massive stars rapidly change their masses through strong stellar winds and mass transfer in binary systems. The latter aspect is important for populations of…”
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The Art of Modeling Stellar Mergers and the Case of the B[e] Supergiant R4 in the Small Magellanic Cloud
Published in The Astrophysical journal (01-09-2020)“…Most massive stars exchange mass with a companion, leading to evolution which is altered drastically from that expected of stars in isolation. Such systems…”
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The MiMeS survey of magnetism in massive stars: magnetic properties of the O-type star population
Published in Monthly notices of the Royal Astronomical Society (11-11-2019)“…ABSTRACT In this paper, we describe an analysis of the MiMeS (Magnetism in Massive Stars) survey of O-type stars to explore the range of dipolar field…”
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