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researcher

Y. K. Ng

4 papers hereh-index 138 citations6 works total

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

author position
  • sole author3
  • middle author1

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

fields
  • astro-ph3
  • astro-ph.GA1
same name
  • Y. K. Ng — 9 papers, h 5
  • Y. K. Ng — 1 paper, h 1

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
19972014
most citedMC^2: Galaxy Imaging and Redshift Analysis of the Merging Cluster CIZA J2242.8+5301

46 citations · 47 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.GA2014★ 46 cited

MC^2: Galaxy Imaging and Redshift Analysis of the Merging Cluster CIZA J2242.8+5301

William A. Dawson, M. James Jee, Andra Stroe +7

X-ray and radio observations of CIZA J2242.8+5301 suggest that it is a major cluster merger. Despite being well studied in the X-ray, and radio, little has been presented on the cl…

astro-ph1998

Are there carbon stars in the Bulge ?

Y. K. Ng

The bulge carbon stars have been a mystery since their discovery, because they are about 2.5mag too faint to be regarded as genuine AGB stars, if located inside the metal-rich bulg…

astro-ph1998

Are the Bulge C-stars related to the Sagittarius dwarf galaxy? II. Metallicity -- a link with the Galactic disc

Y. K. Ng

The photometric estimate of the metallicity and the age of the Azzopardi et al. (1991, A&AS 88, 265) carbon stars (Ng 1997, A&A 328, 211) is revised to respectively Z~0.004 and ~0.…

astro-ph1997★ 1 cited

Are the Bulge C-stars in the Sagittarius dwarf Galaxy ?

Y. K. Ng

Part of the mystery around the Bulge carbon stars from Azzopardi et al. (1991) is solved, if they are related to the Sagittarius dwarf galaxy. The carbon stars are in that case not…

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