Pulsars (rapidly spinning neutron stars) emit beams of intense radiation in the radio part of the electromagnetic spectrum. How these beams are generated remains one of the unsolved mysteries in astrophysics. By studying the pulse-to-pulse variations in their radiation using multiple telescopes simultaneously, we can piece together a three-dimensional map of the intense environment surrounding these compact objects. The quasi-stable structures we observe in their radiation contain important clues to how the emission is generated
Millisecond pulsars are highly sought-after targets for timing-array experiments that aim to detect ...
There has been much progress in detecting and understanding high-energy (∼1 keV-10 GeV) radiation fr...
We present a non-radial oscillation model that can successfully reproduce many properties of driftin...
Pulsars, rapidly rotating neutron stars, are ideal for studying high-energy physics, yet their mecha...
Pulsating aurora is a frequently occurring phenomenon generally believed to occur mainly in the afte...
The double pulsar, PSR J0737-3039A/B, is a unique binary system in which both neutron stars have bee...
Refraction of pulsar radiation by electron density irregularities in the interstellar medium sometim...
Compact Objects (Neutron Stars) form in the last moments of a star\u27s life, during the violent eve...
Pulsars are highly magnetized fast rotating neutron stars producing a pulsed radiation. This thesis ...
Magnetars are a class of highly magnetized, slowly rotating neutron stars, only a small fraction of ...
Contains fulltext : 36190.pdf (publisher's version ) (Open Access)This thesis cons...
We report on the discovery of consecutive bright radio pulses from the Vela pulsar, a new phenomenon...
Almost 50 years after radio pulsars were discovered in 1967, our understanding of these objects rema...
Pulsating aurora, a common phenomenon in the polar night sky, offers a unique opportunity to study t...
observation of the first pulsar discovered by the search which formed the basis for my Ph.D. thesis....
Millisecond pulsars are highly sought-after targets for timing-array experiments that aim to detect ...
There has been much progress in detecting and understanding high-energy (∼1 keV-10 GeV) radiation fr...
We present a non-radial oscillation model that can successfully reproduce many properties of driftin...
Pulsars, rapidly rotating neutron stars, are ideal for studying high-energy physics, yet their mecha...
Pulsating aurora is a frequently occurring phenomenon generally believed to occur mainly in the afte...
The double pulsar, PSR J0737-3039A/B, is a unique binary system in which both neutron stars have bee...
Refraction of pulsar radiation by electron density irregularities in the interstellar medium sometim...
Compact Objects (Neutron Stars) form in the last moments of a star\u27s life, during the violent eve...
Pulsars are highly magnetized fast rotating neutron stars producing a pulsed radiation. This thesis ...
Magnetars are a class of highly magnetized, slowly rotating neutron stars, only a small fraction of ...
Contains fulltext : 36190.pdf (publisher's version ) (Open Access)This thesis cons...
We report on the discovery of consecutive bright radio pulses from the Vela pulsar, a new phenomenon...
Almost 50 years after radio pulsars were discovered in 1967, our understanding of these objects rema...
Pulsating aurora, a common phenomenon in the polar night sky, offers a unique opportunity to study t...
observation of the first pulsar discovered by the search which formed the basis for my Ph.D. thesis....
Millisecond pulsars are highly sought-after targets for timing-array experiments that aim to detect ...
There has been much progress in detecting and understanding high-energy (∼1 keV-10 GeV) radiation fr...
We present a non-radial oscillation model that can successfully reproduce many properties of driftin...
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