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L. Kaper

4 papers here

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

author position
  • first author1
  • middle author3

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

fields
  • astro-ph4
ORCID 0000-0001-8025-8981

identity via Semantic Scholar / OpenAlex

most citedLate-epoch optical and near-infrared observations of the GRB000911 afterglow and its host galaxy

33 citations · 34 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph2005★ 33 cited

Late-epoch optical and near-infrared observations of the GRB000911 afterglow and its host galaxy

N. Masetti, E. Palazzi, E. Pian +28

We present the results of an optical and near-infrared (NIR) monitoring campaign of the counterpart of Gamma-Ray Burst (GRB) 000911, located at redshift z=1.06, from 5 days to more…

astro-ph2005

Massive Stars and their Compact Remnants in High-mass X-ray Binaries

L. Kaper, A. van der Meer

In a high-mass X-ray binary (HMXB) a massive star interacts with a neutron-star or black-hole companion in various ways. The gravitational interaction enables the measurement of fu…

astro-ph2004★ 1 cited

Far Ultraviolet observations of the High Mass X-ray Binary 4U1700-37/HD153919

R. C. Iping, G. Sonneborn, L. Kaper +1

The high-mass X-ray binary 4U1700-37/HD153919 has been observed with FUSE to study the effect of the X-ray source on the stellar wind of the primary. Phase dependent changes in the…

astro-ph2004

Phase-dependent changes in the wind lines in the HMXRB's SMC X-1 and 4U1700-37

R. C. Iping, G. Sonneborn, L. Kaper +1

The High Mass X-ray Binaries (HMXRB's) SMC X-1 and 4U1700-37 have been observed with FUSE to study the effect of the X-ray source on the stellar wind of the primary. In both system…

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