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researcher

Chenyu He

3 papers here

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

author position
  • first author2
  • middle author1

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

fields
  • astro-ph.SR3
ORCID 0000-0001-9131-6956

identity via Semantic Scholar / OpenAlex

most citedThe role of binarity and stellar rotation in the split main sequence of NGC 2422

16 citations · 27 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.SR2023

The role of tidal interactions in the formation of slowly rotating early-type stars in young star clusters

Chenyu He, Chengyuan Li, Weijia Sun +9

The split main sequences found in the colour-magnitude diagrams of star clusters younger than ~600 Myr are suggested to be caused by the dichotomy of stellar rotation rates of uppe…

astro-ph.SR2023★ 11 cited

On the origin of the split main sequences of the young massive cluster NGC 1856

Li Wang, Chengyuan Li, Long Wang +2

The detection of split main sequences (MSs) associated with young clusters (≲600 Myr) has caught lots of attention. A prevailing scenario is that a bimodality of stellar r…

astro-ph.SR2022★ 16 cited

The role of binarity and stellar rotation in the split main sequence of NGC 2422

Chenyu He, Weijia Sun, Chengyuan Li +8

In addition to the extended main-sequence turnoffs widely found in young and intermediate-age (~ 600 Myr-2 Gyr-old) star clusters, some younger clusters even exhibit split main seq…

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