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researcher

S. Srinivasan

57 papers hereh-index 303.2k citations117 works total

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

author position
  • sole author1
  • first author5
  • middle author36
  • last author9

Across the 51 of 57 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR29
  • astro-ph.GA16
  • astro-ph.CO9
  • astro-ph1
  • astro-ph.HE1
  • astro-ph.IM1
same name
  • 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
  • S. Srinivasan — 8 papers

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
20082023
most citedThe global gas and dust budget of the Large Magellanic Cloud: AGB stars and supernovae, and the impact on the ISM evolution

226 citations · 2.7k across the 57 of their papers we have counts for

collaborators
Showing 2021Show all

3 papers · 1 filter

astro-ph.SR2021★ 13 cited

A Census of Thermally-Pulsing AGB stars in the Andromeda Galaxy and a First Estimate of their Contribution to the Global Dust Budget

Steven R. Goldman, Martha L. Boyer, Julianne Dalcanton +5

We present a near-complete catalog of the metal-rich population of Thermally-Pulsing Asymptotic Giant Branch stars in the northwest quadrant of M31. This metal-rich sample compleme…

astro-ph.GA2021

The Nearby Evolved Stars Survey II: Constructing a volume-limited sample and first results from the James Clerk Maxwell Telescope

P. Scicluna, F. Kemper, I. McDonald +89

The Nearby Evolved Stars Survey (NESS) is a volume-complete sample of ∼850 Galactic evolved stars within 3\,kpc at (sub-)mm wavelengths, observed in the CO J= (2−1) and…

astro-ph.GA2021

A Core Mass Function Indistinguishable from the Salpeter Stellar Initial Mass Function Using 1000 au Resolution ALMA Observations

Genaro Suárez, Roberto Galván-Madrid, Luis Aguilar +4

We present the core mass function (CMF) of the massive star-forming clump G33.92+0.11 using 1.3 mm observations obtained with the Atacama Large Millimeter/submillimeter Array (ALMA…

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