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S. Sigurdsson

61 papers hereh-index 477.6k citations193 works total

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

author position
  • sole author4
  • first author3
  • middle author29
  • last author20

Across the 56 of 61 papers where every author was matched, so the position is known.

fields
  • astro-ph42
  • astro-ph.HE5
  • astro-ph.EP4
  • astro-ph.GA4
  • astro-ph.CO2
  • astro-ph.SR2
same name
  • S. Sigurdsson — 1 paper
  • S. Sigurdsson — 1 paper, h 59

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
19942025
most citedExotic Earths: Forming Habitable Worlds with Giant Planet Migration

229 citations · 1.9k across the 37 of their papers we have counts for

collaborators
Showing 2003 · astro-phShow all

4 papers · 2 filters

astro-ph2003★ 2 cited

Simulating the Early Evolution of the Hard X-Ray Properties of a Young Stellar Population

M. S. Sipior, M. Eracleous, S. Sigurdsson

We present an X-ray binary population synthesis model, and use it to simulate the evolution of X-ray binaries formed in a burst of star formation of duration 20 Myr and star-format…

astro-ph2003

A Young White Dwarf Companion to Pulsar 1620-26: Evidence for Early Planet Formation

Steinn Sigurdsson, Harvey B. Richer, Brad M. Hansen +2

The pulsar B1620-26 has two companions, one of stellar mass and one of planetary mass. We detected the stellar companion using Hubble Space Telescope observations. The color and ma…

astro-ph2003

Survival of Terrestrial Planets in the Presence of Giant Planet Migration

Avi M. Mandell, Steinn Sigurdsson

The presence of ``Hot Jupiters'', Jovian mass planets with very short orbital periods orbiting nearby main sequence stars, has been proposed to be primarily due to the orbital migr…

astro-ph2003

Adiabatic Growth of Massive Black Holes

Steinn Sigurdsson

We discuss the process of adiabatic growth of central black holes in the presence of a stationary, pre-existing distribution of collisionless stars. Within the limitations of the a…

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