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researcher

T. Rauch

135 papers hereh-index 272.5k citations314 works total

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

author position
  • sole author8
  • first author11
  • middle author63
  • last author19

Across the 101 of 135 papers where every author was matched, so the position is known.

fields
  • astro-ph74
  • astro-ph.SR48
  • astro-ph.IM6
  • astro-ph.HE3
  • physics.ins-det2
  • astro-ph.EP1
same name
  • T. Rauch — 21 papers, h 9
  • T. Rauch — 20 papers
  • T. Rauch — 13 papers, h 13
  • T. Rauch — 5 papers, h 5
  • T. Rauch — 3 papers, h 2
  • T. Rauch — 2 papers

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
19962022
most citedA grid of synthetic ionizing spectra for very hot compact stars from NLTE model atmospheres

215 citations · 1.9k across the 135 of their papers we have counts for

collaborators
Showing 2019 · astro-ph.SRShow all

3 papers · 2 filters

astro-ph.SR2019★ 21 cited

First discovery of trans-iron elements in a DAO-type white dwarf (BD−22∘3467)

L. Löbling, M. A. Maney, T. Rauch +4

We have identified 484 lines of the trans-iron elements (TIEs) Zn, Ga, Ge, Se, Br, Kr, Sr, Zr, Mo, In, Te, I, Xe, and Ba, for the first time in the ultraviolet spectrum of a DAO-ty…

astro-ph.SR2019★ 10 cited

Two's company, three's a crowd: SALT reveals the likely triple nature of the nucleus of the extreme abundance discrepancy factor planetary nebula Sp 3

B. Miszalski, R. Manick, T. Rauch +3

The substantial number of binary central stars of planetary nebulae (CSPNe) now known (∼50) has revealed a strong connection between binarity and some morphological features i…

astro-ph.SR2019★ 17 cited

Spectral analysis of the hybrid PG 1159-type central stars of the planetary nebulae Abell 43 and NGC 7094

L. Löbling, T. Rauch, M. M. Miller Bertolami +5

Stellar post asymptotic giant branch (post-AGB) evolution can be completely altered by a final thermal pulse (FTP) which may occur when the star is still leaving the AGB (AFTP), at…

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