CO observations reveal molecular clumps at SS 433 X-ray jet re-brightening sites, providing evidence that jet-cloud shocks enhance nonthermal X-ray emission via turbulence and magnetic field amplification.
Title resolution pending
4 Pith papers cite this work. Polarity classification is still indexing.
4
Pith papers citing it
years
2026 4verdicts
UNVERDICTED 4representative citing papers
First ALMA detection of hot cores in RX J1713.7-3946 shows column density ratios of organics, deuterated species, and S/N-bearing molecules indistinguishable from normal hot cores, attributed to recent exposure or magnetic shielding.
Molecular and atomic gas at velocities near -32 and -55 km/s shows spatial correspondence with the TeV gamma-ray shell around Westerlund 1, supporting hadronic cosmic-ray production with total proton energy approximately 6 x 10^49 erg.
Fermi-LAT data show Vela Jr GeV emission matches the H.E.S.S. shell template with index 1.77, and a hybrid model statistically outperforms pure leptonic for the broadband SED.
citing papers explorer
-
Discovery of CO Clouds Associated with the X-ray Jets of SS 433: Evidence for Shock-Cloud Interaction Enhancing Nonthermal X-ray Emission
CO observations reveal molecular clumps at SS 433 X-ray jet re-brightening sites, providing evidence that jet-cloud shocks enhance nonthermal X-ray emission via turbulence and magnetic field amplification.
-
Survival of Molecular Complexity under Recent Supernova Feedback: Detection of Hot Cores in RX J1713.7-3946
First ALMA detection of hot cores in RX J1713.7-3946 shows column density ratios of organics, deuterated species, and S/N-bearing molecules indistinguishable from normal hot cores, attributed to recent exposure or magnetic shielding.
-
Discovery of Molecular and Atomic Gas associated with HESS J1646-458 (Westerlund 1): Spatial TeV Gamma-Ray and Interstellar Proton Correspondence
Molecular and atomic gas at velocities near -32 and -55 km/s shows spatial correspondence with the TeV gamma-ray shell around Westerlund 1, supporting hadronic cosmic-ray production with total proton energy approximately 6 x 10^49 erg.
-
GeV gamma-ray emission in the field of the shell-type supernova remnant Vela Jr revisited
Fermi-LAT data show Vela Jr GeV emission matches the H.E.S.S. shell template with index 1.77, and a hybrid model statistically outperforms pure leptonic for the broadband SED.