Search Results - "Bohlsen, Terry"
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An investigation of the photometric variability of confirmed and candidate Galactic Be stars using ASAS-3 data
Published in Monthly notices of the Royal Astronomical Society (21-09-2018)Get full text
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NuSTAR Detection of X-Rays Concurrent with Gamma-Rays in the Nova V5855 Sgr
Published in The Astrophysical journal (10-02-2019)“…We report the first detection of hard (>10 keV) X-ray emission simultaneous with gamma-rays in a nova eruption. Observations of the nova V5855 Sgr carried out…”
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An investigation of four chemically peculiar stars with photometric periods below 12 h
Published in Monthly notices of the Royal Astronomical Society (01-04-2017)“…We present an investigation of three chemically peculiar (CP) stars and one CP star candidate that exhibit photometric periods below 12 h. New spectroscopic…”
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The Long-term Spectral Changes of Eta Carinae: Are they Caused by a Dissipating Occulter as Indicated by cmfgen Models?
Published in The Astrophysical journal (01-09-2023)“…Eta Carinae ( η Car) exhibits a unique set of P Cygni profiles with both broad and narrow components. Over many decades, the spectrum has changed—there has…”
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A Detailed Observational Analysis of V1324 Sco, the Most Gamma-Ray-luminous Classical Nova to Date
Published in The Astrophysical journal (10-01-2018)“…It has recently been discovered that some, if not all, classical novae emit GeV gamma-rays during outburst, but the mechanisms involved in the production…”
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Erratum: “A Detailed Observational Analysis of V1324 Sco, the Most Gamma-Ray-luminous Classical Nova to Date” (2018, ApJ, 852, 108)
Published in The Astrophysical journal (01-11-2020)Get full text
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The ambiguous transient ASASSN-17hx. A possible nova-impostor
Published 31-01-2020“…A&A 635, A115 (2020) Some transients, although classified as novae based on their maximum and early decline optical spectra, cast doubts on their true nature…”
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An investigation of the photometric variability of confirmed and candidate Galactic Be stars using ASAS-3 data
Published 30-05-2018“…We present an investigation of a large sample of confirmed (N=233) and candidate (N=54) Galactic classical Be stars (mean V magnitude range of 6.4 to 12.6…”
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QZ Carinae Orbit of the Two Binary Pairs
Published 11-02-2020“…We present an updated O-C diagram of the light-time variations of the eclipsing binary (component B) in the system QZ Carinae as it moves in the long-period…”
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An Investigation of Four Chemically Peculiar Stars with Photometric Periods below 12 Hours
Published 14-12-2016“…We present an investigation of three chemically peculiar (CP) stars and one CP star candidate which exhibit photometric periods below 12 hours. New…”
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NuSTAR Detection of X-rays Concurrent with Gamma Rays in the Nova V5855 Sgr
Published 31-12-2018“…We report the first detection of hard (>10 keV) X-ray emission simultaneous with gamma rays in a nova eruption. Observations of the nova V5855 Sgr carried out…”
Get full text
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ST Chamaeleontis and BP Coronae Australis: Two Southern Dwarf Novae Confirmed as Z Cam Stars
Published 02-02-2014“…Z Camelopardalis (Z Cam) stars are a subset of dwarf novae distinguished by the occurrence of standstills, periods of relative constant brightness one to one…”
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The variability of the BRITE-est Wolf-Rayet binary, $\gamma^2$ Velorum I. Photometric and spectroscopic evidence for colliding winds
Published 11-07-2017“…We report on the first multi-color precision light curve of the bright Wolf-Rayet binary $\gamma^2$ Velorum, obtained over six months with the nanosatellites…”
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A Detailed Observational Analysis of V1324 Sco, the Most Gamma-Ray Luminous Classical Nova to Date
Published 21-11-2017“…It has recently been discovered that some, if not all, classical novae emit GeV gamma rays during outburst, but the mechanisms involved in the production of…”
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BRITE-Constellation high-precision time-dependent photometry of the early-O-type supergiant $\zeta$ Puppis unveils the photospheric drivers of its small- and large-scale wind structures
Published 23-10-2017“…From $5.5$ months of dual-band optical photometric monitoring at the $1$ mmag level, BRITE-Constellation has revealed two simultaneous types of variability in…”
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