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P. M. Sánchez-Alarcón

2 papers here

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

author position
  • middle author1
  • last author1

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

fields
  • astro-ph.GA1
  • astro-ph.HE1
ORCID 0000-0002-6278-9233

identity via Semantic Scholar / OpenAlex

most citedEvidence for globular cluster collapse after a dwarf-dwarf merger: A potential nuclear star cluster in formation

9 citations · 9 across the 2 of their papers we have counts for

collaborators

2 papers

astro-ph.HE2024

Detection of an intranight optical hard-lag with colour variability in blazar PKS 0735+178

Callum McCall, Helen E. Jermak, Iain A. Steele +3

Blazars are a highly variable subclass of active galactic nuclei that have been observed to vary significantly during a single night. This intranight variability remains a debated…

astro-ph.GA2023★ 9 cited

Evidence for globular cluster collapse after a dwarf-dwarf merger: A potential nuclear star cluster in formation

J. Román, P. M. Sánchez-Alarcón, J. H. Knapen +1

Direct observational evidence for the creation of nuclear star clusters (NSCs) is needed to support the proposed scenarios for their formation. We analysed the dwarf galaxy UGC 734…

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