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L. Waters

17 papers hereh-index 161.1k citations23 works total

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

author position
  • middle author14
  • last author1

Across the 15 of 17 papers where every author was matched, so the position is known.

fields
  • astro-ph12
  • astro-ph.GA3
  • astro-ph.SR2
same name
  • L. Waters — 59 papers, h 39
  • L. Waters — 26 papers, h 22
  • L. Waters — 23 papers, h 33
  • L. Waters — 21 papers, h 10
  • L. Waters — 19 papers, h 21
  • L. Waters — 14 papers, h 17

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
20012026
most citedCrystalline silicate dust around evolved stars II. The crystalline silicate complexes

199 citations · 1.2k across the 16 of their papers we have counts for

collaborators
Showing 2001Show all

3 papers · 1 filter

astro-ph2001★ 52 cited

The discovery of the "21" micron and "30" micron emission features in Planetary Nebulae with Wolf-Rayet central stars

S. Hony, L. B. F. M. Waters, A. G. G. M. Tielens

We report the discovery of the "21" micron and "30" micron features in the planetary nebulae around the hydrogen-deficient stars HD 826 and HD 158269. The carriers of these feature…

astro-ph2001★ 82 cited

The complete ISO spectrum of NGC 6302

F. J. Molster, T. L. Lim, R. J. Sylvester +6

We present the combined Infrared Space Observatory Short-Wavelength Spectrometer and Long-Wavelength Spectrometer 2.4--197 micron spectrum of the Planetary Nebula NGC 6302 which co…

astro-ph2001★ 92 cited

Crystallinity versus mass-loss rate in Asymptotic Giant Branch stars

F. Kemper, L. B. F. M. Waters, A. de Koter +1

Infrared Space Observatory (ISO) observations have shown that O-rich Asymptotic Giant Branch (AGB) stars exhibit crystalline silicate features in their spectra only if their mass-l…

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