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K. Heng

170 papers hereh-index 5811.3k citations293 works total

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

author position
  • sole author5
  • first author16
  • middle author89
  • last author46

Across the 156 of 170 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP139
  • astro-ph.SR10
  • astro-ph9
  • astro-ph.IM5
  • astro-ph.HE4
  • astro-ph.GA2
same name
  • K. Heng — 6 papers, h 4
  • K. Heng — 4 papers, h 1
  • K. Heng — 3 papers, h 5
  • K. Heng — 2 papers, h 4
  • K. Heng — 1 paper, h 6
  • K. Heng — 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
20052026
most citedCan we constrain interior structure of rocky exoplanets from mass and radius measurements?

353 citations · 6.9k across the 126 of their papers we have counts for

collaborators
Showing 2007 · astro-phShow all

4 papers · 2 filters

astro-ph2007★ 28 cited

Probing Elemental Abundances in SNR 1987A Using XMM-Newton

Kevin Heng, Frank Haberl, Bernd Aschenbach +1

We report on the latest (2007 Jan) observations of supernova remnant (SNR) 1987A from the XMM-Newton mission. Since the 2003 May observations of Haberl et al. (2006), 11 emission l…

astro-ph2007★ 29 cited

Broad Lyman-Alpha Emission from Supernova Remnants in Young Galaxies

Kevin Heng, Rashid Sunyaev

Charge transfer (or exchange) reactions between hydrogen atoms and protons in collisionless shocks of supernova remnants (SNRs) are a natural way of producing broad Balmer, Lyman a…

astro-ph2007★ 34 cited

The Transition Zone in Balmer-Dominated Shocks

Kevin Heng, Matthew van Adelsberg, Richard McCray +1

We examine the structure of the post-shock region in supernova remnants (SNRs). The ``shock transition zone'' is set up by charge transfer and ionization events between atoms and i…

astro-ph2007★ 1 cited

The Reverse Shock of SNR 1987A

Kevin Heng

The reverse shock of supernova remnant (SNR) 1987A emits in H-alpha and Ly-alpha, and comes in two flavors: surface and interior. The former is due to direct, impact excitation of…

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