Results 71 to 80 of about 37,456 (169)

MILAN Sky Survey, a dataset of raw deep sky images captured during one year with a Stellina automated telescope. [PDF]

Data Brief, 2023
Parisot O, Hitzelberger P, Bruneau P, Krebs G, Destruel C, Vandame B.   +5 more
europepmc   +1 more source

High Resolution CO and H2 Molecular Line Imaging of a Cometary Globule in the Helix Nebula

, 2002
We report high resolution imaging of a prominent cometary globule in the Helix nebula in the CO J=1-0 (2.6 mm) and H2 v=1-0 S(1) (2.12 micron) lines. The observations confirm that globules consist of dense condensations of molecular gas embedded in the ...
Dyson J. E., Dyson J. E., Forveille T., J. R. Walsh, Meaburn J., N. Ageorges, Natta A., P. Cox, P. J. Huggins, R. Bachiller, T. Forveille, Walsh J. R.   +11 more
core   +1 more source

Towards an explanation for the 30 Dor (LMC) Honeycomb nebula - the impact of recent observations and spectral analysis

, 2010
The unique Honeycomb nebula, most likely a peculiar supernova remnant, lies in 30 Doradus in the Large Magellanic Cloud. Due to its proximity to SN1987A, it has been serendipitously and intentionally observed at many wavelengths.
Boumis, Chu, Chu, Chu, Crotts, Dennerl, Dunne, E. Harvey, Fabrika, Feng, Goudis, Haberl, J. Meaburn, Lazendic, M. P. Redman, Meaburn, Meaburn, Meaburn, Meaburn, Meaburn, Meaburn, P. Boumis, Payne, Redman, Russel, Russell, Sabbadin, Smith, Steffen, Steffen, Wang, Whitehead   +31 more
core   +1 more source

Detection of shocked atomic gas in the Kleinmann-Low nebula [PDF]

The 63 micrometer (3)p(1)-(3)P(2) fine structure line emission of neutral atomic oxygen at the center of the Orion nebula with a resolution of 30" is presented. There are three main emission peaks.
Crawford, M. K., Genzel, R., Hollenbach, D. J., Townes, C. H., Watson, F. M., Werner, M.   +5 more
core   +1 more source

C^+ distribution around S1 in rho Ophiuchi

, 2018
We analyze a [C II] 158 micron map obtained with the L2 GREAT receiver on SOFIA of the emission/reflection nebula illuminated by the early B star S1 in the rho-OphA cloud core.
Chambers, E., Guesten, R., Mookerjea, B., Sandell, G., Vacca, W.   +4 more
core   +1 more source

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

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

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

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

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