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The Radio Emission Model

A Subrelativistic Shock Model for the Radio Emission of SN 1998bw

A Subrelativistic Shock Model for the Radio Emission of SN 1998bw

... The emission spectrum predicted by our model for mono-energetic electrons provides an excellent fit to the observational radio data of SN1998bw (see ...of model predictions to data around the ...

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A Model for the Flaring Radio Emission in the Double Pulsar System J0737-3039

A Model for the Flaring Radio Emission in the Double Pulsar System J0737-3039

... pulsed radio flux from pulsar B brightens considerably during two portions of each ...at radio frequencies within an altitude of ∼ 10 8 cm. The radio photons then travel through B’s magnetosphere and ...

5

Diffuse radio emission in MACS J1752.0+4440.

Diffuse radio emission in MACS J1752.0+4440.

... This requires additional observations which are currently obtained and the resulting spectral and polarization study will be presented in a forthcoming paper (Bonafede et al., MNRAS, submitted). The presence of a ...

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Physics of radio emission in gamma-ray pulsars

Physics of radio emission in gamma-ray pulsars

... dipole model, contain a number of additional ingredients, such as the global electric current, the accelerating electric field, ...of radio waves in the force-free magnetosphere, and what it may imply for ...

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Auroral radio emission and absorption of medium frequency radio waves observed in Iceland

Auroral radio emission and absorption of medium frequency radio waves observed in Iceland

... auroral radio emissions in the polar iono- sphere, the ARS system was installed at the Husafell station in ...MF radio emissions, it is necessary to examine the nature of ionospheric ...

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CiteSeerX — A Model for the Offsets between X-ray and Radio Emission from Large Scale AGN Jets

CiteSeerX — A Model for the Offsets between X-ray and Radio Emission from Large Scale AGN Jets

... shell model, we find that the offsets between the peaks of X-ray, optical and radio brightness distributions observed for many cases are basically explained with this ...while radio emission ...

7

The ionization of the emission-line gas in young radio galaxies

The ionization of the emission-line gas in young radio galaxies

... nuclear emission lines in compact radio sources are often broad, with asymmetric profiles requiring mul- tiple Gaussian components to model ...nuclear emission lines for all sources in our ...

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The Relationship Between the Radio and Gamma Ray Emission of Blazars

The Relationship Between the Radio and Gamma Ray Emission of Blazars

... the model used for the light curves has motivated some researchers to search for model-independent significance ...appropriate model for the light ...a model independent ...

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Simulating radio emission from low mass stars

Simulating radio emission from low mass stars

... this radio emission was ECM, then our model should be able to reproduce the radio light ...The radio spectrum shown in Figure 2 is the result of assuming every fi eld line that satis fi ...

8

Is lightning a possible source of the radio emission on HAT P 11b?

Is lightning a possible source of the radio emission on HAT P 11b?

... 2011). We assume that the atmosphere is hydrogen rich, and the atmospheric gas of HAT-P-11b is at roughly solar metal- licity with respect to C, N and O, i.e. that the primordial concentrations of these elements in ...

5

Diffuse radio emission at low frequencies in merging galaxy clusters

Diffuse radio emission at low frequencies in merging galaxy clusters

... of radio halos, radio relics, and radio ...diffuse radio emission and their characterization has signi- ficantly ...of radio halos with ongoing merger events is very well ...

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Characterizing the radio continuum emission from intense starburst galaxies

Characterizing the radio continuum emission from intense starburst galaxies

... (synchrotron) emission components that comprise the radio continuum of galaxies represent unique, dust-free measures of star forma- tion rates ...future radio surveys. We disentangle the thermal and ...

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Upper limits on gravitational wave emission from 78 radio pulsars

Upper limits on gravitational wave emission from 78 radio pulsars

... For all except P ulsar 9 the h 0 values were reduced by a ∼ half, with P ulsar 9 being so strong that its ampli- tude was reduced by a factor of ∼ 20. These signals were injected for the second half of the run from 8 th ...

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THE MORPHOLOGY OF THE EMISSION-LINE REGION OF COMPACT STEEP-SPECTRUM RADIO SOURCES1

THE MORPHOLOGY OF THE EMISSION-LINE REGION OF COMPACT STEEP-SPECTRUM RADIO SOURCES1

... the radio emission extends over more than 1A and the HST resolution is such that a detailed comparison can be made between radio and optical ...the radio lobes, possibly tracing the path of ...

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Upper limits on gravitational wave emission from 78 radio pulsars

Upper limits on gravitational wave emission from 78 radio pulsars

...  i 2 F  t k ; h 0 cose i2 0 ; (3.2) is the gravitational wave signal model evaluated at t k , the time corresponding to the kth heterodyned sample. In Ref. [ 3 ] the value of m j was fixed at 30 to give 30 ...

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Upper limits on gravitational wave emission from 78 radio pulsars

Upper limits on gravitational wave emission from 78 radio pulsars

... known radio pulsars, the Crab pulsar has of- ten been considered one of the most promising sources of gravitational ...glitch model favoured for the Crab pulsar involves a change in the pulsar ellipticity, ...

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Weak and compact radio emission in early high mass star forming regions  II  The nature of the radio sources

Weak and compact radio emission in early high mass star forming regions II The nature of the radio sources

... 70 radio sources reported in Paper I. These radio sources were observed using the VLA at 6 and ...previous radio continuum detection or a relatively weak detection at the 1 mJy ...gas emission ...

23

Radio-quiet quasars in the VIDEO survey : evidence for AGN-powered radio emission at S-1.4 GHz

Radio-quiet quasars in the VIDEO survey : evidence for AGN-powered radio emission at S-1.4 GHz<1 mJy

... the radio map included, to ensure a fair comparison between model and ...the radio emission is due to accretion, then the power-law used to describe the brightness-weighted number counts above ...

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FCC Radio emission Requirements in Utah

FCC Radio emission Requirements in Utah

... B) Confirm consumer eligibility by relying upon access to a state database and/or notice of eligibility from the state Lifeline administrator prior to enrolling a con[r] ...

6

Observations of pulsar radio emission with microsecond resolution

Observations of pulsar radio emission with microsecond resolution

... Indeed an auto-correlation analysis of these thirteen channels does not show any significant periodicity (Chapter 9). The vertical scale of the thirteen traces in the Figure has been s[r] ...

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