most citedOptical observations of the fast nova V1674 Herculis

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6 papers

astro-ph.HE20261 cited

Optical observations of the fast nova V1674 Herculis

Neeraj Singh Rawat, L. S. Sonith, U. S. Kamath +3

We present the evolution of optical spectra and lightcurves of the fast nova V1674 Herculis during 150 days past its eruption. Using the post-eruption AAVSO light curve, we have ca…

astro-ph.HE2026

A NICER and AstroSat view of the neutron star low-mass X-ray binary 1A 1246-588

Vaidehi Poojyam, Vikas Mistry, Yash Bhargava +2

Neutron star (NS) low-mass X-ray binary (LMXB) systems depict a variety of X-ray spectral and timing features, which can be useful to probe the accretion-ejection mechanism in the…

astro-ph.HE2026

A joint MeerKAT and Parkes view of Omega Centauri: New TRAPUM Searches and Pulsar Timing

Miquel Colom i Bernadich, Shi Dai, Federico Abbate +27

Millisecond pulsars (MSPs) are powerful probes of globular clusters (GCs), tracing stellar evolution, cluster dynamics, and the local gravitational potential. We investigate the MS…

astro-ph.HE2025

Infrared Synchrotron Emission in the Soft State of GX 339-4 and the Mid-Infrared/X-ray Luminosity Plane of Black Hole X-ray Binaries

P. Gandhi, D. M. Russell, M. C. Baglio +33

Progress in understanding the growth of accreting black holes remains hampered by a lack of sensitive coordinated multiwavelength observations. In particular, the mid-infrared (MIR…

astro-ph.HE2025

Probing the accreting millisecond X-ray pulsar SAX J1808.4-3658 using the evolution of its spectral and aperiodic timing properties

Aman Kaushik, Yash Bhargava, Sudip Bhattacharyya +1

Understanding accretion components in neutron star (NS) low mass X-ray binary (LMXB) systems is important to probe fundamental aspects of accretion mechanism and evolution of the s…

astro-ph.HE2025

X-ray and Radio Campaign of the Z-source GX 340+0 II: the X-ray polarization in the normal branch

Yash Bhargava, Thomas D. Russell, Mason Ng +11

We present the first X-ray polarization measurement of the neutron star low-mass X-ray binary and Z-source, GX 3400, in the normal branch (NB) using a 200 ks observation with th…