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researcher

K. Biazzo

17 papers hereh-index 441 citations19 works total

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

author position
  • middle author14
  • last author2

Across the 16 of 17 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR10
  • astro-ph.GA3
  • astro-ph.EP2
  • astro-ph.IM2
same name
  • K. Biazzo — 166 papers, h 39
  • K. Biazzo — 23 papers, h 11
  • K. Biazzo — 6 papers
  • K. Biazzo — 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
20222026
most citedProtoplanetary discs around sun-like stars appear to live longer when the metallicity is low

14 citations · 21 across the 17 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

3 papers · 1 filter

astro-ph.GA2026

The Stellar Population of NGC 346 in the Small Magellanic Cloud with JWST

J. Jaspers, P. Kavanagh, G. De Marchi +13

NGC 346 is a massive star-forming region located at a distance of ∼62 kpc, in the Small Magellanic Cloud (SMC). Due to its low metallicity (Z ∼1/5 Z⊙​), it is an…

astro-ph.GA2025

A Mid-Infrared Spectroscopic Study of Young Stellar Objects in the SMC Region NGC 346: JWST Detects Dust, Accretion, Ices and Outflows

Nolan Habel, Omnarayani Nayak, Patrick J. Kavanagh +13

We present mid-infrared spectroscopic observations of intermediate- to high-mass young stellar objects (YSOs) in the low-metallicity star-forming region NGC 346 located within the…

astro-ph.GA2025

First detection of ices in intermediate-mass young stellar objects beyond the Milky Way

Guido De Marchi, Nolan Habel, Margaret Meixner +15

Using NIRSpec on JWST, we studied a sample of 15 intermediate-mass (1.8-4.1 Msun) young stellar objects (YSOs) previously identified with MIRI photometry in the low-metallicity NGC…

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