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researcher

W. Herbst

44 papers hereh-index 355.2k citations227 works total

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

author position
  • first author13
  • middle author24
  • last author4

Across the 41 of 44 papers where every author was matched, so the position is known.

fields
  • astro-ph23
  • astro-ph.SR17
  • astro-ph.EP4
same name
  • W. Herbst — 11 papers, h 8
  • W. Herbst — 1 paper, h 0

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
20002021
most citedCSI 2264: Simultaneous optical and infrared light curves of young disk-bearing stars in NGC 2264 with CoRoT and Spitzer-- evidence for multiple origins of variability

411 citations · 2.7k across the 44 of their papers we have counts for

collaborators
Showing 2012Show all

3 papers · 1 filter

astro-ph.SR2012★ 62 cited

Locating the Trailing Edge of the Circumbinary Ring in the KH 15D System

Holly L. Capelo, William Herbst, S. K. Leggett +2

Following two years of complete occultation of both stars by its opaque circumbinary ring, the binary T Tauri star KH 15D has abruptly brightened again during apastron phases, reac…

astro-ph.SR2012★ 13 cited

An unusual very low-mass high-amplitude pre-main sequence periodic variable

Maria V. Rodriguez-Ledesma, Reinhard Mundt, Mansur Ibrahimov +5

We have investigated the nature of the variability of CHS7797, an unusual periodic variable in the Orion Nebula Cluster. An extensive I-band photometric data set of CHS7797 was com…

astro-ph.SR2012★ 20 cited

Complex Variability of the Hα Emission Line Profile of the T Tauri Binary System KH 15D: The Influence of Orbital Phase, Occultation by the Circumbinary Disk, and Accretion Phenomenae

Catrina M. Hamilton, Christopher M. Johns-Krull, Reinhard Mundt +2

We have obtained 48 high resolution echelle spectra of the pre-main sequence eclipsing binary system KH~15D (V582 Mon, P = 48.37 d, e ∼ 0.6, MA​ = 0.6 M⊙​, M$_{B…

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