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researcher

B. Hansen

59 papers hereh-index 458.6k citations171 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • sole author10
  • first author8
  • middle author27
  • last author13

Across the 58 of 59 papers where every author was matched, so the position is known.

fields
  • astro-ph28
  • astro-ph.EP26
  • astro-ph.SR4
  • physics.chem-ph1
same name
  • B. Hansen — 6 papers, h 6
  • B. Hansen — 5 papers, h 28
  • B. Hansen — 2 papers, h 1
  • B. Hansen — 2 papers, h 52
  • B. Hansen — 1 paper, h 1
  • B. Hansen — 1 paper, h 1

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
19982023
most citedThe Chemical Composition of an Extrasolar Minor Planet

338 citations · 2.5k across the 43 of their papers we have counts for

collaborators
Showing 2005 · astro-phShow all

4 papers · 2 filters

astro-ph2005

A Spitzer Search for Infrared Excesses around Massive Young White Dwarfs

Brad M. S. Hansen, Shri Kulkarni, Sloane Wiktorowicz

We examine 14 hot white dwarfs for signs of infrared excess using the Spitzer Space Telescope. Twelve of the objects are massive white dwarfs which have been suggested to be the re…

astro-ph2005

White Dwarfs in NGC 6791: Avoiding the Helium Flash

Brad Hansen

We propose that the anomalously bright white dwarf luminosity function observed in NGC 6791 (Bedin et al 2005) is the consequence of the formation of 0.5 Msun white dwarfs with Hel…

astro-ph2005

On the Dayside Thermal Emission of Hot Jupiters

S. Seager, L. J. Richardson, B. M. S. Hansen +3

We discuss atmosphere models of HD209458b in light of the recent day-side flux measurement of HD209458b's secondary eclipse by Spitzer-MIPS at 24 microns. In addition, we present a…

astro-ph2005

The white dwarf cooling sequence in NGC 6791

L. R. Bedin, M. Salaris, G. Piotto +5

In the old, populous, and metal-rich open cluster NGC 6791 we have used deep HST/ACS images to track the white dwarf cooling sequence down to m_F606W~28.5. The white dwarf luminosi…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.