Radio Pulsar Phenomenology: What can we learn from pulsar profiles?

More documents

Recommendations

Info

Basic Observables and Derivables. II.MeasureDM, RM, Tscatt, HI absorptionDeriveInterstellar medium densityInterstellar medium magnetic fieldInterstellar medium turbulence<strong>Pulsar</strong> distances Global picture of Galaxy structure
Basic Observables and Derivables. II.MeasureDM, RM, TscattJohnston et al. 2005Loehmer et al. 2004Image: Reiner Beck
Page 1 and 2: Radio Pulsar Phenomenology:What can
Page 3: Basic Observables and Derivables. I
Page 19 and 20: Kramer et al. 2006Image: NASAVerbie
Page 21 and 22: Basic Observables and Derivables. V
Page 23 and 24: Pulsar geometry and therotating vec
Page 25 and 26: The Rotating Vector Model (RVM) for
Page 37 and 38: α = 30, β = -1.7α = 86, β = -3.
Page 39 and 40: Mapping the magnetosphere• We can
Page 41 and 42: Beam modelof Lyne &ManchesterIn a n
Page 43 and 44: Young pulsarstudy ofJohnston &Weisb
Page 45 and 46: Polarization and the P-Pdot diagram
Page 47 and 48: Orthogonal RotatorsWeltevrede & Wri
Page 49 and 50: Summary• The integrated profiles

Radio Pulsar Phenomenology: What can we learn from pulsar profiles?

Create successful ePaper yourself

Delete template?

Save as template?