Results 111 to 120 of about 1,887,037 (257)

JWST Observations of the Ring Nebula (NGC 6720). III. A Dusty Disk around Its Central Star

open access: yesThe Astrophysical Journal
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

Some like it cold: molecular emission and effective dust temperatures of dense cores in the Pipe Nebula [PDF]

open access: bronze, 2014
Jan Forbrich   +6 more
openalex   +1 more source

Thermal Dust Emission from Proplyds, Unresolved Disks, and Shocks in the Orion Nebula [PDF]

open access: bronze, 2005
Nathan Smith   +4 more
openalex   +1 more source

The Morphology and Kinematics of a Giant, Symmetric Nebula around a Radio-loud Quasar 3C 57: Extended Rotating Gas or Biconical Outflows?

open access: yesThe Astrophysical Journal
Gas flows between galaxies and the circumgalactic medium play a crucial role in galaxy evolution. When ionized by a quasar, these gas flows can be directly traced as giant nebulae. We present a study of a giant nebula around a radio-loud quasar, 3C 57 at
Zhuoqi (Will) Liu   +13 more
doaj   +1 more source

Precise Measurements of TeV Halos around Geminga and Monogem Pulsars with HAWC

open access: yesThe Astrophysical Journal
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
doaj   +1 more source

A Morphokinematic Study of the Enigmatic Emission Nebula NGC 6164/5 Surrounding the Magnetic O-type Star HD 148937

open access: yesThe Astrophysical Journal
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
doaj   +1 more source

Very-high-energy γ-Ray Emission from Young Massive Star Clusters in the Large Magellanic Cloud

open access: yesThe Astrophysical Journal Letters
The Tarantula Nebula in the Large Magellanic Cloud is known for its high star formation activity. At its center lies the young massive star cluster R136, providing a significant amount of the energy that makes the nebula shine so brightly at many ...
F. Aharonian   +132 more
doaj   +1 more source

Large-scale Wind-driven Structures in the Orion Nebula

open access: yesThe Astronomical Journal
A study of [C ii ] 158 μ m and H i 21 cm spectroscopic images plus high-velocity-resolution optical and ultraviolet spectra has shown the structure of the Orion Nebula to be different from that found from the study of those data separately.
C. R. O’Dell, N. P. Abel
doaj   +1 more source

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