He
Patrick Hartigan
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Modeling Ionized Gas in the Small Magellanic Cloud: The Wolf–Rayet Nebula N76
We present Cloudy modeling of infrared emission lines in the Wolf–Rayet (WR) nebula N76 caused by one of the most luminous and hottest WR stars in the low metallicity Small Magellanic Cloud.
Elizabeth Tarantino +7 more
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Iron Fluorescent Line Emission from Young Stellar Objects in the Orion Nebula [PDF]
Masahiro Tsujimoto +7 more
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Spectral energy distribution modeling of broadband emission in the pulsar wind nebula 3C 58 [PDF]
Seungjong Kim, Hongjun An
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Evidence of an Energetic Magnetar Powering 1LHAASO J0500+4454
We investigate the origin of the unidentified, extended TeV source 1LHAASO J0500+4454, considering three possible origins: cosmic rays interacting with a molecular cloud (MC), particles accelerated in a currently undetected supernova remnant (SNR), and ...
J. A. J. Alford +3 more
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Relationship between CH3OD Abundance and Temperature in the Orion KL Nebula. [PDF]
Wilkins OH, Blake GA.
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Suzaku Observation of Diffuse X-Ray Emission from the Carina Nebula [PDF]
Kenji Hamaguchi +11 more
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Discovery of spectacular quasar-driven superbubbles in red quasars. [PDF]
Shen L +9 more
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The braking index of PSR B0540−69 and the associated pulsar wind nebula emission after spin-down rate transition [PDF]
Ling‐Jun Wang +8 more
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GeV Gamma-Ray Emission from Pulsar Wind Nebula HESS J1356-645 with Fermi-Large Area Telescope [PDF]
Xi Liu +4 more
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