Results 251 to 260 of about 2,108,053 (297)
Intrapulse multimodal four-wave sum mixing in the visible range from high contrast index grating with PMMA layer. [PDF]
Light Sci ApplFranceschini P +10 more
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High-Yield Room-Temperature Aryl <sup>211</sup>At Radiolabeling via Redox-Activated Column-Shipped <sup>211</sup>At. [PDF]
ACS Org Inorg AuPerera JS +8 more
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Radio continuum and CO emission in star-forming galaxies [PDF]
Astronomy and Astrophysics, 2002 We combine the radio continuum images from the NRAO VLA Sky Survey with the CO-line observations from the extragalactic CO survey of the Five College Radio Astronomy Observatory to study the relationship between molecular gas and the star formation rate within the disks of 180 spiral galaxies at 45" resolution. We find a tight correlation between these
Matteo Murgia +2 more
exaly +7 more sources
Radio continuum emission from a tidal dwarf galaxy [PDF]
Monthly Notices of the Royal Astronomical SocietyABSTRACT Tidal dwarf galaxies (TDGs) form in the debris of galaxy mergers, making them ideal testbeds for investigating star formation in an extreme environment. We present radio continuum EVLA observations spanning 1–2 GHz of the interacting system Arp 94, which contains the TDG J1023+1952.
Miguel Querejeta +2 more
exaly +5 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 +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 +2 more
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Detection of continuum radio emission associated with Geminga [PDF]
Monthly Notices of the Royal Astronomical Society: Letters, 2011 Abstract A deep Very Large Array observation of the Geminga pulsar field led to the discovery, at a higher than 10σ significance level, of radio emission trailing the neutron star proper motion. This ∼10 arcsec long radio feature, detected with a flux of ∼0.4 mJy at 4.8 GHz, is marginally displaced (2.7 ± 1.8 arcsec) from the pulsar ...
Andrea Possenti +2 more
exaly +3 more sources
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Spotless Flares and the Associated Radio Continuum Emission
Solar Physics, 1987.
Ruždjak, Vladimir +5 more
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Models of Uranian continuum radio emission
Journal of Geophysical Research: Space Physics, 1987The 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 +4 more
openaire +1 more source
The ultraviolet continuum emission of radio galaxies
AIP Conference Proceedings, 1997This poster presents the UV continuum emission (in the range from 1400 to 3700 A) of radio galaxies (with redshift ranging from 0.01 to 0.1 and radio powers ranging from 1025 to 1027 Watts/Hz). The sample of radio galaxies were compiled by searching the Hubble Space Telescope (HST) archives for images taken with the Faint Object Camera (FOC) prior to ...
Esther L. Zirbel, Stefi A. Baum
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