Showing 1–20 of 131 results
/ Date/ Name
Aug 7, 2020The disintegrating old open cluster Czernik 3Sep 28, 2010Multi-wavelength polarimetric study towards the open cluster NGC 1893May 24, 2022Azimuthal transverse single-spin asymmetries of inclusive jets and identified hadrons within jets from polarized $pp$ collisions at $\sqrt{s}$ = 200 GeVApr 20, 2012Contribution of Acoustic Losses in the Quality Factor of a Micromechanical ResonatorSep 15, 2012Star formation activity in the Galactic H II region Sh2-297Jan 24, 2020Variable stars in the Sh 2-170 HII regionMar 9, 2021Longitudinal double-spin asymmetry for inclusive jet and dijet production in polarized proton collisions at $\sqrt{s}=200$ GeVMar 24, 2021Invariant Jet Mass Measurements in $pp$ Collisions at $\sqrt{s} = 200$ GeV at RHICMay 31, 2021Measurement of the Sixth-Order Cumulant of Net-Proton Multiplicity Distributions in Au+Au Collisions at $\sqrt{s_{\rm NN}}=$ 27, 54.4, and 200 GeV at RHICMar 31, 2014The molecular complex associated with the Galactic HII region Sh2-90: a possible site of triggered star formationOct 31, 2002Interstellar extinction in the open clusters towards galactic longitude around 130 degreesOct 16, 2002Identification of 13 Cepheids and 333 Other Variables in M31Feb 9, 2001The extraordinarily bright optical afterglow of GRB 991208 and its host galaxyMar 1, 1999Spectral Energy Distributions and Light Curves of GRB 990123 and its AfterglowAug 30, 2007A multiwavelength study of Galactic HII region Sh2-294Nov 18, 2023Production of Protons and Light Nuclei in Au+Au Collisions at $\sqrt{s_{\mathrm{NN}}}$ = 3 GeV with the STAR DetectorJan 26, 2023Energy Dependence of Intermittency for Charged Hadrons in Au+Au Collisions at RHICJul 22, 2025Energy Independence of the Collins Asymmetry in $p^{\uparrow}p$ CollisionsDec 8, 2021Light Nuclei Collectivity from $\sqrt{s_{\rm NN}}$ = 3 GeV Au+Au Collisions at RHICSep 24, 2022Higher-Order Cumulants and Correlation Functions of Proton Multiplicity Distributions in $\sqrt{s_{\mathrm{NN}}}$ = 3 GeV Au+Au Collisions at the RHIC STAR Experiment