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Gajendra Pandey

4 papers hereh-index 11 citations4 works total

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

author position
  • last author4

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

fields
  • astro-ph.SR4
same name
  • Gajendra Pandey — 2 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

most citedDetection of Enhanced Germanium in a New Cool Extreme Helium Star A 980: Insights and Implications

2 citations · 2 across the 2 of their papers we have counts for

collaborators

4 papers

astro-ph.SR2025

Photospheric Helium Abundance in Cool Giants -- A Comprehensive Study

B. P. Hema, Gajendra Pandey

High-resolution optical spectra of sixteen red giants, two early asymptotic giant branch (AGB) stars, and two supergiants, having no/minimal to super lithium (Li)-rich abundances,…

astro-ph.SR2024★ 2 cited

Detection of Enhanced Germanium in a New Cool Extreme Helium Star A 980: Insights and Implications

Ajay Kumar Saini, Gajendra Pandey

A fine abundance analysis of a recently discovered hydrogen-deficient carbon (HdC) star, A 980, is presented. Based on the observed high-resolution optical spectrum, we ascertain t…

astro-ph.SR2024

Helium Abundance of the Sun: A Spectroscopic Analysis

Satyajeet Moharana, B. P. Hema, Gajendra Pandey

Determining the He/H ratio in cool stars presents a fundamental astrophysical challenge. While this ratio is established for hot O and B stars, its extrapolation to cool stars rema…

astro-ph.SR2024

Measuring Hydrogen-to-Helium Ratio in Cool Stars

B. P. Hema, Gajendra Pandey

Conventionally, the helium-to-hydrogen ratio for the stars are adopted to be 0.1, as standard, unless, the stars are severely deficient in hydrogen like in RCB-class, or the stars'…

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