9.8k citations
- Tata Institute of Fundamental ResearchIN259 papers
- Eötvös Loránd UniversityHU243 papers
- Massachusetts Institute of TechnologyUS233 papers
- University of Maryland, College ParkUS233 papers
- California Institute of TechnologyUS232 papers
- University of FloridaUS230 papers
- Seoul National UniversityKR228 papers
- Tsinghua UniversityCN227 papers
- Sapienza University of RomeIT226 papers
- HUN-REN Wigner Research Centre for PhysicsHU225 papers
- University of GenoaIT225 papers
- University of PerugiaIT225 papers
921 papers
Magnetic Fields in Massive Star-forming Regions (MagMaR). IX. Radiative Torque Alignment and Disruption in NGC6334I
Vineet Rawat, Thiem Hoang, Patricio Sanhueza +18
Intense radiation from high-mass stars is expected to significantly affect dust grain alignment and evolution through RAdiative Torques (RATs). We investigate this effect in a mass…
Early Exploration of the Scientific Discovery Space for the Habitable Worlds Observatory
Courtney D. Dressing, Danica Adams, Evelyne Alecian +324
The Habitable Worlds Observatory (HWO) is a future NASA flagship mission concept identified by the Astro2020 Decadal Survey as the highest priority for large space missions. HWO sh…
Multi-Wavelength Diagnostics of Pre-Flare Evolution with Aditya-L1: From the Solar Chromosphere to the Corona
Adithya H. N., Sreejith Padinhatteeri, Soumya Roy +13
The pre-flare phase of solar flares provides important insight into the processes that drive active regions toward instability. We investigate chromospheric pre-flare activity usin…
Identifying mobility edge from finite temperature spectral form factor
Basudha Roy, Anandamohan Ghosh, Adway Kumar Das
The spectral form factor (SFF) is a measure of energy correlations and has been widely used to identify the transition from the ergodic to the localized phase in interacting many-b…
Iron Fluorescence in X-class Solar Flares: Aditya-L1/SoLEXS Observations
Abhilash R. Sarwade, K. Sankarasubramanian, Monoj Bug +5
Iron fluorescence is produced by the irradiation of the solar photosphere by coronal X-rays during flares. This study presents the first comprehensive analysis of iron K fluores…
A Parameterized YSO Accretion Disk Model with Increasing Accretion Rate: Predicted Outburst Lightcurves
Gautam Das, Lynne A. Hillenbrand, Adolfo S. Carvalho
A sub-class among Young Stellar Objects (YSOs), known as FU Ori type stars, undergo sudden rises in luminosity by several orders of magnitude on timescales of a few months to a few…