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S. Srinivasan

4 papers hereh-index 11 citations6 works total

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

author position
  • middle author2

Across the 2 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR3
  • astro-ph.GA1
same name
  • S. Srinivasan — 57 papers, h 30
  • S. Srinivasan — 55 papers, h 28
  • S. Srinivasan — 19 papers, h 15
  • S. Srinivasan — 14 papers, h 7
  • S. Srinivasan — 13 papers, h 20
  • S. Srinivasan — 13 papers, h 15

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 citedThe ALMA detection of CO rotational line emission in AGB stars in the Large Magellanic Cloud

27 citations · 28 across the 4 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

3 papers · 1 filter

astro-ph.SR2025

Discovery of SiC and Iron Dust Around AGB Stars in the very Metal-Poor Sextans A Dwarf Galaxy with JWST: Implications for Dust Production at High Redshift

M. L. Boyer, G. C. Sloan, A. Nanni +23

Low-resolution infrared spectroscopy from JWST confirms the presence of SiC and likely metallic iron dust around asymptotic giant branch (AGB) stars in the Sextans A dwarf galaxy,…

astro-ph.SR2025

The Nearby Evolved Stars Survey (NESS) V: properties of volume-limited samples of Galactic evolved stars

I. McDonald, S. Srinivasan, P. Scicluna +23

We provide a meta-study of the statistical and individual properties of two volume-complete sets of evolved stars in the Solar Neighbourhood: (1) 852 stars from the Nearby Evolved…

astro-ph.SR2016★ 27 cited

The ALMA detection of CO rotational line emission in AGB stars in the Large Magellanic Cloud

M. A. T. Groenewegen, W. H. T. Vlemmings, P. Marigo +21

Context: Low- and intermediate-mass stars lose most of their stellar mass at the end of their lives on the asymptotic giant branch (AGB). Determining gas and dust mass-loss rates (…

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