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W. Fischer

4 papers hereh-index 272.8k citations111 works total

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

author position
  • first author1
  • middle author2
  • last author1

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph4
same name
  • W. Fischer — 2 papers, h 8
  • W. Fischer — 1 paper
  • W. Fischer — 1 paper, h 19
  • W. Fischer — 1 paper, h 8

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
20032008
most citedProbing T Tauri Accretion and Outflow with 1 Micron Spectroscopy

248 citations · 440 across the 3 of their papers we have counts for

collaborators

4 papers

astro-ph2008★ 80 cited

Redshifted Absorption at He I 10830 as a Probe of the Accretion Geometry of T Tauri Stars

William Fischer, John Kwan, Suzan Edwards +1

We probe the geometry of magnetospheric accretion in classical T Tauri stars by modeling red absorption at He I 10830 via scattering of the stellar and veiling continua. Under the…

astro-ph2006★ 112 cited

Modeling T Tauri Winds from He I 10830 Profiles

John Kwan, Suzan Edwards, William Fischer

The high opacity of He I 10830 makes it an exceptionally sensitive probe of the inner wind geometry of accreting T Tauri stars. In this line blueshifted absorption below the contin…

astro-ph2006★ 248 cited

Probing T Tauri Accretion and Outflow with 1 Micron Spectroscopy

Suzan Edwards, William Fischer, Lynne Hillenbrand +1

In a high dispersion 1 micron survey of 39 classical T Tauri stars veiling is detected in 80%, and He I 10830 and Pgamma line emission in 97% of the stars. On average, the 1 micron…

astro-ph2003

He I 10830 as a Probe of Winds in Accreting Young Stars

S. Edwards, W. Fischer, J. Kwan +2

He I 10830 profiles acquired with Keck's NIRSPEC for 6 young low mass stars with high disk accretion rates (AS 353A, DG Tau, DL Tau, DR Tau, HL Tau and SVS 13) provide new insight…

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