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B. H. Dunlap

Researcher at University of North Carolina at Chapel Hill

Publications -  30
Citations -  1278

B. H. Dunlap is an academic researcher from University of North Carolina at Chapel Hill. The author has contributed to research in topics: White dwarf & Light curve. The author has an hindex of 15, co-authored 30 publications receiving 1046 citations. Previous affiliations of B. H. Dunlap include University of Texas at Austin & Association of Universities for Research in Astronomy.

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The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. III. Optical and UV Spectra of a Blue Kilonova from Fast Polar Ejecta

TL;DR: In this paper, optical and ultraviolet spectra of the binary neutron star merger GW170817 were obtained nightly between 1.5 and 9.5 days post-merger, using the SOAR and Magellan telescopes.
Journal ArticleDOI

The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. III. Optical and UV Spectra of a Blue Kilonova From Fast Polar Ejecta

TL;DR: In this paper, optical and ultraviolet spectra of the binary neutron star merger GW170817 were obtained nightly between 1.5 and 9.5 days post-merger, using the SOAR and Magellan telescopes.
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Evryscope science: exploring the potential of all-sky gigapixel-scale telescopes

TL;DR: The Evryscope as mentioned in this paper is an under-construction 780 MPix telescope which covers 8,660 square degrees in each two-minute exposure; each night, 18,400 square degrees will be continuously observed for an average of approximately 6 hours.
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Analysis of Helium-rich White Dwarfs Polluted by Heavy Elements in the Gaia Era

TL;DR: In this article, a homogeneous analysis of 1023 DBZ/DZ(A) and 319 DQ white dwarf stars taken from the Montreal White Dwarf Database is presented, which represents a significant increase over the previous comprehensive studies on these types of objects.
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Core crystallization and pile-up in the cooling sequence of evolving white dwarfs

TL;DR: In this article, the authors report the presence of a pile-up in the cooling sequence of evolving white dwarfs within 100 parsecs of the Sun, determined using photometry and parallax data from the Gaia satellite.