Results 251 to 260 of about 2,146,207 (296)

A nearby dark molecular cloud in the Local Bubble revealed via H₂ fluorescence. [PDF]

Nat Astron
Burkhart B, Dharmawardena TE, Bialy S, Haworth TJ, Cruz Aguirre F, Jo YS, Andersson BG, Chung H, Edelstein J, Grenier I, Hamden ET, Han W, Hoadley K, Lee MY, Min KW, Müller T, Pattle K, Peek JEG, Pleiss G, Schiminovich D, Seon KI, Wilson AG, Zucker C.   +22 more
europepmc   +1 more source

PSMA-Targeted Radioligand Therapy Beyond the Post-Taxane Setting: A Review of Evidence Across the Prostate Cancer Spectrum. [PDF]

Cancers (Basel)
Wang K, Hassanbhai DH, Teo RYA, Ong CSH, Lai KW, Koo SX, Yam WL, Tung JYM.   +7 more
europepmc   +1 more source

Analysis of Niobium and Stainless Steel Electropolishing Solutions by Laser-Induced Breakdown Spectroscopy Using a Porous Silicon Substrate and a Non-Contact Pretreatment. [PDF]

Materials (Basel)
Matsumoto A, Takeda Y, Kuroda K, Torigoe H, Sugita Y, Shimazu Y, Nii K, Ida Y, Yae S.   +8 more
europepmc   +1 more source

Discovery of H 3 + and infrared aurorae at Neptune with JWST. [PDF]

Nat Astron
Melin H, Moore L, Fletcher LN, Hammel HB, O'Donoghue J, Stallard TS, Milam SN, Roman M, King ORT, Rowe-Gurney N, Thomas EE, Wang R, Tiranti PI, Harkett J, Knowles KL.   +14 more
europepmc   +1 more source

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The Infrared and Radio-Continuum Emission of the Galactic Disk

Nature, 1987
In 1983 the Infrared Astronomical Satellite (IRAS) surveyed the sky in four wavebands in the far infrared (FIR). One of the products of this survey1 is a detailed picture with an angular resolution of ∼4 arc min of the infrared emission of the interstellar dust in the galactic plane.
J L Osborne
exaly   +2 more sources

Properties of the Radio Continuum Emission From Interacting Galaxies

Nature, 1973
SEVERAL interacting galaxies have been observed recently in different programmes using the Westerbork Synthesis Radio Telescope at 21 cm wavelength (beamwidth 24 s × 24 s cosec δ). We give here a compilation of the data in order to examine the morphology, strength, and the frequency of occurrence of the radio emission from these interacting systems.
Ronald Ekers, G K Miley, B F Burke
exaly   +2 more sources

Characterizing the Radio Continuum Emission From Intense Starburst Galaxies [PDF]

Monthly Notices of the Royal Astronomical Society, 2016
The intrinsic thermal (free–free) and non-thermal (synchrotron) emission components that comprise the radio continuum of galaxies represent unique, dust-free measures of star formation rates (SFR). Such high SFR galaxies will dominate the deepest current
Tim J Galvin, Miroslav Filipovic, Guillaume Drouart   +2 more
exaly   +4 more sources

The Tiered Radio Extragalactic Continuum (T-RECS) Simulation II: H I Emission and Continuum-H i Cross-Correlation [PDF]

Monthly Notices of the Royal Astronomical Society, 2023
In this paper we extend the Tiered Radio Extragalactic Continuum Simulation (T-RECS) to include HI emission. The HI T-RECS model is based on the most recent HI mass function estimates, combined with prescriptions to convert HI mass to total integrated HI
Philippa Hartley, Matteo Bonato, Gianfranco de Zotti   +2 more
exaly   +2 more sources

Spotless Flares and the Associated Radio Continuum Emission

Solar Physics, 1987
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Ruždjak, Vladimir, M. Messerotti, M. Nonino, A. Schroll, Vršnak, Bojan, P. Zlobec   +5 more
openaire   +2 more sources

Models of Uranian continuum radio emission

Journal of Geophysical Research: Space Physics, 1987
The Uranian kilometric emissions detected by the Voyager 2 Planetary Radio Astronomy (PRA) experiment during the January 1986 encounter comprise two distinct types of emission: bursts and continuum. The bursts have been treated by Evans et al. (this issue). This paper considers the continuum emissions. The continuum emissions comprised four components:
Joseph H. Romig, David R. Evans, Constance B. Sawyer, Andrea E. Schweitzer, James W. Warwick   +4 more
openaire   +1 more source