Detection of Vibrational Emissions from the Helium Hydride Ion (HeH+) in the Planetary Nebula NGC 7027 [PDF]
David A. Neufeld +5 more
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Discovery of TeV gamma-ray emission from the pulsar wind nebula 3C 58 by MAGIC
The pulsar wind nebula (PWN) 3C 58 is one of the historical very-high-energy (VHE; E>100 GeV) gamma-ray source candidates. It has been compared to the Crab Nebula due to their morphological similarities.
López-Coto Rubén
doaj +1 more source
Progenitor stars of long gamma-ray bursts (GRBs) could be surrounded by a significant and complex nebula structure lying at a parsec-scale distance. After the initial release of energy from the GRB jet, the jet will interact with this nebula environment.
Asaf Pe’er, Felix Ryde
doaj +1 more source
Thermal Dust Emission from Proplyds, Unresolved Disks, and Shocks in the Orion Nebula [PDF]
Nathan Smith +9 more
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JWST Observations of the Ring Nebula (NGC 6720). III. A Dusty Disk around Its Central Star
The planetary nebula NGC 6720, also known as the “Ring Nebula,” is one of the most iconic examples of nearby planetary nebulae whose morphologies present a challenge to our theoretical understanding of the processes that govern the deaths of most stars ...
Raghvendra Sahai +18 more
doaj +1 more source
Hard X-ray emission from the eastern jet of SS 433 powering the W50\n `Manatee' nebula: Evidence for particle re-acceleration [PDF]
Samar Safi‐Harb +14 more
openalex +1 more source
Possible Pulsed Gamma Ray Emission from the Crab Nebula Pulsar [PDF]
W. N. Charman, George Michael White
openalex +1 more source
Investigating the multiband non-thermal emission of the 100 TeV source eHWC J2019+368 with a pulsar wind nebula scenario [PDF]
Jun Fang, Lu Wen, Huan Yu, S. Z. Chen
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Precise Measurements of TeV Halos around Geminga and Monogem Pulsars with HAWC
We present the most precise measurements to date for the spatial extension and energy spectrum of the γ -ray region between a pulsar’s wind nebula and the interstellar medium, better known as the halo, present around Geminga and PSR B0656+14 (Monogem ...
A. Albert +94 more
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HD 148937 is a peculiar massive star (Of?p) with a strong magnetic field (1 kG). The hourglass-shaped emission nebula NGC 6164/5 surrounds this star. This nebula is presumed to originate from episodic mass-loss events of the central O-type star, but the ...
Beomdu Lim +3 more
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