Results 141 to 150 of about 143,052 (287)

Relationship between CH₃OD Abundance and Temperature in the Orion KL Nebula. [PDF]

J Phys Chem A, 2022
Wilkins OH, Blake GA.
europepmc   +1 more source

Neutral hydrogen in the Andromeda Nebula –I. H I emission in the south-west region of the nebula [PDF]

, 1980
S. C. Unwin
openalex   +1 more source

The Molecular Exoskeleton of the Ring-like Planetary Nebula NGC 3132

The Astrophysical Journal
We present Submillimeter Array (SMA) mapping of ^12 CO J = 2 → 1, ^13 CO J = 2 → 1, and CN N = 2 → 1 emission from the ring-like planetary nebula NGC 3132, one of the subjects of JWST Early Release Observation near-infrared imaging.
Joel H. Kastner, David J. Wilner, Paula Moraga Baez, Jesse Bublitz, Orsola De Marco, Raghvendra Sahai, Al Wootten   +6 more
doaj   +1 more source

Discovery of spectacular quasar-driven superbubbles in red quasars. [PDF]

Sci Adv, 2023
Shen L, Liu G, He Z, Zakamska NL, Glikman E, Greene JE, Hu W, Mou G, Wylezalek D, Rupke DSN.   +9 more
europepmc   +1 more source

H₂ and HI Emission Line Imaging of the Ring Nebula NGC 6720 [PDF]

, 1989
M. A. Greenhouse, T. L. Hayward, H. A. Thronson   +2 more
openalex   +1 more source

Transient Arh+ Emission In The Crab Nebula

, 2017
N ...
S. Viti, Mile Barlow, Ilse De Looze, F. D. Priestley, I. Jimenez-Serra   +4 more
openaire   +3 more sources

Interactions between Pulsars, Pulsar Nebulae and Supernova Remnants [PDF]

arXiv, 2002
The Crab Nebula is likely to be expanding into freely expanding supernova ejecta, although the energy in the ejecta may be less than is typical for a Type II supernova. Pulsar nebulae much younger than the Crab have not been found and could have different properties. The search for such nebulae through ultraviolet/optical line emission in core collapse
arxiv  

On the role of diffuse emission nebulae in galaxies [PDF]

Symposium - International Astronomical Union, 1958
The emission nebulae, as more or less compact gaseous or gas-and-dust formations, belong to a rather widespread type of population in our Galaxy. Though, for well-known reasons, we are able to penetrate into the depth of the Galaxy no further than 2–3 kpc for H 11 regions, several hundred nebulae have already been recorded (predominantly in the spiral ...
openaire   +1 more source

Detection of companion galaxies around hot dust-obscured hyper-luminous galaxy W0410-0913. [PDF]

Nat Commun, 2022
Ginolfi M, Piconcelli E, Zappacosta L, Jones GC, Pentericci L, Maiolino R, Travascio A, Menci N, Carniani S, Rizzo F, Arrigoni Battaia F, Cantalupo S, De Breuck C, Graziani L, Knudsen K, Laursen P, Mainieri V, Schneider R, Stanley F, Valiante R, Verhamme A.   +20 more
europepmc   +1 more source

Starburst-driven superwinds from infrared galaxies [PDF]

New data is presented that indicate that strong far infrared galaxies commonly have largescale emission line nebulae whose properties are suggestive of mass outflows (superwinds), presumably driven by the high supernova rate associated with the central ...
Armus, Lee, Heckman, Timothy M., Mccarthy, Patrick, Miley, George K., Vanbreugel, Wil   +4 more
core   +1 more source