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N. Lehner

5 papers hereh-index 10559 citations19 works total

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

author position
  • first author2

Across the 2 of 5 papers where every author was matched, so the position is known.

fields
  • astro-ph5
same name
  • N. Lehner — 11 papers, h 37

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
20032006
most citedLow Redshift Intergalactic Absorption Lines in the Spectrum of HE0226-4110

43 citations · 86 across the 2 of their papers we have counts for

collaborators

4 papers

astro-ph2006★ 43 cited

Low Redshift Intergalactic Absorption Lines in the Spectrum of HE0226-4110

N. Lehner, B. D. Savage, B. P. Wakker +2

We present an analysis of the FUSE and STIS E140M spectra of HE0226-4110 (z=0.495). We detect 56 Lyman absorbers and 5 O VI absorbers. The number of intervening O VI systems per un…

astro-ph2005

CaII K observations of QSOs in the line-of-sight to the Magellanic Bridge

J. V. Smoker, F. P. Keenan, H. M. A. Thompson +5

We describe medium-resolution spectroscopic observations taken with the ESO Multi-Mode Instrument in the CaII K line (3933.661 Angstroms) towards 7 QSOs located in the line-of-sigh…

astro-ph2004

Small-Scale Structure of O VI Interstellar Gas in the Direction of the Globular Cluster NGC 6752

N. Lehner, J. C. Howk

In order to study the small-scale structure of the hot interstellar gas, we obtained Far Ultraviolet Spectroscopic Explorer interstellar O VI interstellar absorption spectra of 4 f…

astro-ph2003

FUSE Survey of the Local Interstellar Medium within 200 Parsec

N. Lehner, E. B. Jenkins, C. Gry +3

We present FUSE observations of the interstellar gas toward 30 white dwarf and 1 subdwarf (SdO) stars. These sightlines probe the Local Bubble (LB) and the local interstellar mediu…

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