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D. Jones

4 papers hereh-index 210 citations8 works total

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

author position
  • middle author3

Across the 3 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR3
  • astro-ph.EP1
same name
  • D. Jones — 39 papers, h 21
  • D. Jones — 27 papers, h 93
  • D. Jones — 18 papers, h 35
  • D. Jones — 16 papers, h 23
  • D. Jones — 15 papers, h 42
  • D. Jones — 11 papers, h 11

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

most citedMUSE spectroscopy of the high abundance discrepancy planetary nebula NGC 6153

10 citations · 10 across the 2 of their papers we have counts for

collaborators

4 papers

astro-ph.SR2026

Investigating the electron temperature of [Ar IV] in planetary nebulae using the DESIRED database

J. García-Rojas, E. Reyes-Rodríguez, J. E. Méndez-Delgado +9

(Abridged) We investigate the behaviour of the electron temperature derived from [Ar IV] lines, Te([Ar IV]), in a sample of PNe to characterize the thermal structure of high-excita…

astro-ph.SR2026

Ancient 'ghost' planetary nebulae discovered with amateur telescopes

J. A. Manuel, D. Jones, M. Santander-García +1

As planetary nebulae evolve, they fade and dissipate into the surrounding interstellar medium making them harder to detect. Modern, advanced amateur equipment can help to uncover t…

astro-ph.SR2024★ 10 cited

MUSE spectroscopy of the high abundance discrepancy planetary nebula NGC 6153

V. Gómez-Llanos, J. García-Rojas, C. Morisset +5

(Abridged) The abundance discrepancy problem in planetary nebulae (PNe) has long puzzled astronomers. NGC6153, with its high Abundance Discrepancy Factor (ADF~10), provides an oppo…

astro-ph.EP2024

HD 110067 c has an aligned orbit

J. Zak, H. M. J. Boffin, E. Sedaghati +25

Planetary systems in mean motion resonances hold a special place among the planetary population. They allow us to study planet formation in great detail as dissipative processes ar…

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