215 citations · 830 across the 26 of their papers we have counts for
26 papers
Super-Chandrasekhar white dwarfs by the evolution of magnetized main-sequence stars: New mass-limits from STARS simulation
Zenia Zuraiq, Banibrata Mukhopadhyay, Achal Kumar +4
We explore the time evolution of the magnetized main-sequence stars (MSs) to magnetized non-rotating white dwarfs (WDs) with a series of models, capturing modified Hertzsprung-Russ…
HR-GO II: chemical abundances of low- retrograde dynamically-tagged-groups: Revealing Thamnos as a very metal-poor substructure
Renjing Xie, Zhen Yuan, Haining Li +12
Milky Way halo substructures identified in dynamical space are known to suffer from contamination from the Milky Way in-situ stars, which makes their accreted origins uncertain. We…
Origin of -Poor Very Metal-Poor Stars
S. K. Jeena, Projjwal Banerjee
Among very metal-poor (VMP) stars, -poor VMP (PVMP) stars that have sub-solar values of for Mg and other elements are rare and are thought to have been for…
Can supernova from runaway stars mimic the signs of absorbing `super-virial' gas?
Mukesh Singh Bisht, Projjwal Banerjee, Biman B. Nath +1
The recent detection of large column density absorption lines from highly ionized gas in a few directions through the circumgalactic medium (CGM) of the Milky Way (MW) has been puz…
SDSSJ0018-0939: A Clear Signature of Sub-Chandrasekhar Mass Type 1a Supernova
S. K. Jeena, Projjwal Banerjee
Very metal-poor (VMP) stars () that have sub-solar values of for elements such as Mg, Si, and Ca, are referred to as -poor VMP stars. The…
Origin of LAMOST J1010+2358 Revisited
S. K. Jeena, Projjwal Banerjee
Signature from Pop III massive stars of -- that end their lives as pair-instability supernovae (PISNe) are expected to be seen in very metal-poor (VMP) sta…