activity
20122020
most citedAbundance analyses of the new R Coronae Borealis stars: ASAS-RCB-8 and ASAS-RCB-10

11 citations · 20 across the 3 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2020

Investigation of the Helium Enhancement in a Super Lithium Rich Giant HD 77361

B. P. Hema, Gajendra Pandey

In this work, the helium-enhancement (He-enhancement) in the lithium-rich (Li-rich) K-giant HD 77361 is investigated using the strengths of the MgH band and the MgI lines. The deta…

astro-ph.SR20208 cited

Helium Enhancement in the Metal Rich Red Giants of Omega Centauri

B. P. Hema, Gajendra Pandey, R. L. Kurucz +1

The helium-enriched (He-enriched) metal-rich red giants of Omega Centauri, discovered by Hema and Pandey using the low-resolution spectra from the Vainu Bappu Telescope (VBT) and c…

astro-ph.SR2018

High resolution spectroscopy of the relatively hydrogen-poor metal rich giants in the globular cluster Omega Centauri

B. P. Hema, Gajendra Pandey, R. Srianand

High-resolution optical spectra are analyzed for two of the four metal rich mildly hydrogen-poor or helium-enhanced giants discovered by Hema and Pandey (2014) along with their com…

astro-ph.SR201711 cited

Abundance analyses of the new R Coronae Borealis stars: ASAS-RCB-8 and ASAS-RCB-10

B. P. Hema, Gajendra Pandey, Devika Kamath +3

Abundance analyses of the two newly discovered R Coronae Borealis (RCB) stars ASAS-RCB-8 and ASAS-RCB-10 were conducted using high-resolution optical spectra and model atmospheres.…

astro-ph.SR2016

The hot Gamma-Doradus and Maia stars

L. A. Balona, C. A. Engelbrecht, Yogesh C. Joshi +8

The hot ~Doradus stars have multiple low frequencies characteristic of ~Dor or SPB variables, but are located between the red edge of the SPB and the blue edge of the ~Dor…

astro-ph.SR20121 cited

The Galactic R Coronae Borealis Stars and the Final He-shell Flash Object V4334 Sgr (Sakurai's Object): A Comparison

B. P. Hema, Gajendra Pandey, David L. Lambert

The high resolution optical spectra of H-deficient stars, R Coronae Borealis stars and H-deficient carbon stars are analyzed by synthesizing the C2 Swan bands (0,1), (0,0), and (1,…