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researcher

Na’ama Hallakoun

3 papers here

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

author position
  • middle author1
  • last author2

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR3
ORCID 0000-0002-0430-7793

identity via Semantic Scholar / OpenAlex

activity
20162024
most citedThe binary fraction, separation distribution, and merger rate of white dwarfs from SPY

41 citations · 71 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.SR2024★ 8 cited

Ba Enrichment in Gaia MS+WD Binaries: Tracing s-Process Element Production

Param Rekhi, Sagi Ben-Ami, Na'ama Hallakoun +3

A large population of intermediate-separation binaries, consisting of a main-sequence (MS) star and a white dwarf (WD), has recently emerged from Gaia's third data release (DR3), p…

astro-ph.SR2022★ 22 cited

Hyper-runaway and hypervelocity white dwarf candidates in \textit{Gaia} Data Release 3: possible remnants from Ia/Iax supernova explosions or dynamical encounters

Andrei P. Igoshev, Hagai Perets, Na'ama Hallakoun

Type Ia and other peculiar supernovae (SNe) are thought to originate from the thermonuclear explosions of white dwarfs (WDs). Some of the proposed channels involve the ejection of…

astro-ph.SR2016★ 41 cited

The binary fraction, separation distribution, and merger rate of white dwarfs from SPY

Dan Maoz, Na'ama Hallakoun

From a sample of spectra of 439 white dwarfs (WDs) from the ESO-VLT Supernova-Ia Progenitor surveY (SPY), we measure the maximal changes in radial-velocity (DRVmax) between epochs…

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