Results 61 to 70 of about 608,712 (186)
Discovery of metal line emission from the Red star in IP Peg during outburst maximum [PDF]
Observations of the eclipsing dwarf nova IP Peg during outburst reveal metal lines in emission, such as Mg II 4481 A. Analysis using Doppler tomography locates emission of helium and metal lines on the inner Roche lobe of the secondary star.
Harlaftis, E. T.
core +1 more source
Optimization of photomixers and antennas for continuous-wave terahertz emission [PDF]
We have studied terahertz emission from interdigitated finger photomixers coupled to planar antenna structures. Using both pulsed and continuous-wave excitation, polarization measurements reveal that the antenna design dominates the properties of the
Baker, C. +7 more
core +1 more source
THERMAL EMISSION OF WASP-14b REVEALED WITH THREESPITZERECLIPSES [PDF]
Exoplanet WASP-14b is a highly irradiated, transiting hot Jupiter. Joshi et al. calculate an equilibrium temperature Teq of 1866 K for zero albedo and reemission from the entire planet, a mass of 7.3 +/- 0.5 Jupiter masses and a radius of 1.28 +/- 0.08 Jupiter radii.
Blecic, Jasmina +12 more
openaire +4 more sources
Photometric observations of the radio bright B[e]/X-ray binary CI Cam [PDF]
We present multiwavelength (optical, IR, radio) observations of CI Cam, the optical counterpart to the transient X-ray source XTE J0421+560. Pre-outburst quiescent observations reveal the presence of a dusty envelope around the system.
Clark, J. S. +17 more
core
ORFEUS II and IUE Spectroscopy of EX Hydrae [PDF]
Using ORFEUS-SPAS II FUV spectra, IUE UV spectra, and archival EUVE deep survey photometry, we present a detailed picture of the behavior of the magnetic cataclysmic variable EX Hydrae. Like HUT spectra of this source, the FUV and UV spectra reveal broad
Bath G. T. +12 more
core +2 more sources
Radio emission from a pulsar’s magnetic pole revealed by general relativity [PDF]
General relativity reveals pulsar beams Pulsars are rotating neutron stars that emit beams of radio waves along their magnetic poles, seen as regular pulses if the beam points toward Earth. Desvignes et al. monitored a pulsar for more than a decade, observing how its radio pulses vary.
Gregory Desvignes +9 more
openaire +6 more sources
Extended OH(1720 MHz) Maser Emission from Supernova Remnants
Compact OH(1720 MHz) masers have proven to be excellent signposts for the interaction of supernova remnants with adjacent molecular clouds. Less appreciated has been the weak, extended OH(1720 MHz) emission which accompanies strong compact maser sources.
D. A. Roberts +4 more
core +1 more source
Helioseismic analysis of the solar flare-induced sunquake of 2005 January 15 [PDF]
We report the discovery of one of the most powerful sunquakes detected to date, produced by an X1.2-class solar flare in active region 10720 on 2005 January 15.
Besliu-Ionescu, D. +4 more
core +1 more source
The perovskite light-emitting diodes (PeLEDs) have attracted considerable research interests in recent years due to their decent and tunable optoelectronic characteristics.
Qing Ci +7 more
doaj +1 more source
We measured the angle- and polarization-resolved reflection and photoluminescence spectra of ZnO inverse opals. Significant enhancement of spontaneous emission is observed.
C. López +6 more
core +1 more source

