activity
19992023
most citedInfrared Space Observatory Spectra of R Coronae Borealis Stars. I. Emission Features in the Interval 3 - 25 microns

63 citations · 709 across the 42 of their papers we have counts for

collaborators
Showing astro-phShow all

12 papers · 1 filter

astro-ph2007

Fluorine in R Coronae Borealis and Extreme Helium Stars

Gajendra Pandey, David L. Lambert, N. Kameswara Rao

Neutral fluorine lines are identified in the optical spectra of several R Coronae Borealis stars (RCBs) at maximum light. These lines provide the first measurement of the fluorine…

astro-ph2007★ 62 cited

Fluorine in R Coronae Borealis Stars

Gajendra Pandey, David L. Lambert, N. Kameswara Rao

Neutral fluorine (F I) lines are identified in the optical spectra of several R Coronae Borealis stars (RCBs) at maximum light. These lines provide the first measurement of the flu…

astro-ph2006★ 33 cited

Discovery of Fluorine in Cool Extreme Helium Stars

Gajendra Pandey

Neutral fluorine (F I) lines are identified in the optical spectra of cool EHe stars. These are the first identification of F I lines in a star's spectrum, and provide the first me…

astro-ph2006★ 16 cited

Abundance analysis of cool extreme helium star: LSS 3378

Gajendra Pandey, Bacham E. Reddy

Abundance analysis of the cool extreme helium (EHe) star LSS 3378 is presented. The abundance analysis is done using LTE line formation and LTE model atmospheres constructed for EH…

astro-ph2005★ 46 cited

An analysis of ultraviolet spectra of Extreme Helium Stars and new clues to their origins

Gajendra Pandey, David L. Lambert, C. Simon Jeffery +1

Abundances of about 18 elements including the heavy elements Y and Zr are determined from Hubble Space Telescope Space Telescope Imaging Spectrograph ultraviolet spectra of seven e…

astro-ph2004★ 16 cited

The R Coronae Borealis stars - carbon abundances from forbidden carbon lines

Gajendra Pandey, David L. Lambert, N. Kameswara Rao +3

Spectra of several R Coronae Borealis (RCB) stars at maximum light were examined for the [C I] 9850 A and 8727 A absorption lines. The 9850 A line is variously blended with a Fe II…