Secular and orbital changes in emission from J0737-3039 system

Andrea Possenti; Marta Burgay; Michael Kramer; Andrew Lyne; Maura McLaughlin; Duncan Lorimer; Ingrid Stairs; Robert Ferdman; Dick Manchester; George Hobbs; Fernando Camilo; Nichi D'Amico; Paulo Freire; John Sarkissian

doi:10.1063/1.2774915

Secular and orbital changes in emission from J0737-3039 system

Andrea Possenti, Marta Burgay, Michael Kramer, Andrew Lyne, Maura McLaughlin, Duncan Lorimer, Ingrid Stairs, Robert Ferdman, Dick Manchester, George Hobbs, Fernando Camilo, Nichi D'Amico, Paulo Freire, John Sarkissian

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Abstract

The double-pulsar J0737-3039 is not only the most promising system for testing general relativity, but appears a unique laboratory for investigating the so far unaccessible pulsar magnetosphere and the mechanism for radio emission. In fact, the very high orbital inclination gives the possibility of using the radio beams from pulsar A as a probe for investigating the region close to the surface of pulsar B, while relativistic effects modify the system geometry in a timescale suitable for comparing predictions of various models with observation. We present the status of the multi-wavelength observations performed in the 3 years since the discovery and discuss short and long term perspectives for the study of the magnetosphere of pulsar B.

Original language	English
Title of host publication	AIP Conference Proceedings: Multicolored Landscape of Compact Objects and their Explosive Origins
Editors	L Angelo Antonelli, Gian Luca Israel, Luciano Piersanti, Amedeo Tornambe, Luciano Burderi, Tiziana Di Salvo, Fabrizio Fiore, Giorgio Matt, Maria Teresa Menna
Publisher	American Institute of Physics
Chapter	591
Volume	924
ISBN (Print)	978-0-7354-0434-2
DOIs	https://doi.org/10.1063/1.2774915
Publication status	Published - 21 Aug 2007
Externally published	Yes
Event	Conference on Multicolored Landscape of Compact Objects and Their Explosive Origins - Cefalu, Italy Duration: 11 Jun 2006 → 18 Jun 2006

Publication series

Name	AIP Conference Proceedings
Publisher	American Institute of Physics
Volume	924
ISSN (Print)	0094-243X

Conference

Conference	Conference on Multicolored Landscape of Compact Objects and Their Explosive Origins
Country/Territory	Italy
City	Cefalu
Period	11/06/06 → 18/06/06

Keywords

neutron star
pulsar : individual (J0737-3039A, J0737-3039B)
DOUBLE PULSAR
RADIO-EMISSION
MODULATION
ECLIPSES

Access to Document

10.1063/1.2774915

Cite this

Possenti, A., Burgay, M., Kramer, M., Lyne, A., McLaughlin, M., Lorimer, D., Stairs, I., Ferdman, R., Manchester, D., Hobbs, G., Camilo, F., D'Amico, N., Freire, P., & Sarkissian, J. (2007). Secular and orbital changes in emission from J0737-3039 system. In L. A. Antonelli, G. L. Israel, L. Piersanti, A. Tornambe, L. Burderi, T. Di Salvo, F. Fiore, G. Matt, & M. T. Menna (Eds.), AIP Conference Proceedings: Multicolored Landscape of Compact Objects and their Explosive Origins (Vol. 924). (AIP Conference Proceedings; Vol. 924). American Institute of Physics. https://doi.org/10.1063/1.2774915

Possenti, Andrea ; Burgay, Marta ; Kramer, Michael ; Lyne, Andrew ; McLaughlin, Maura ; Lorimer, Duncan ; Stairs, Ingrid ; Ferdman, Robert ; Manchester, Dick ; Hobbs, George ; Camilo, Fernando ; D'Amico, Nichi ; Freire, Paulo ; Sarkissian, John. / Secular and orbital changes in emission from J0737-3039 system. AIP Conference Proceedings: Multicolored Landscape of Compact Objects and their Explosive Origins. editor / L Angelo Antonelli ; Gian Luca Israel ; Luciano Piersanti ; Amedeo Tornambe ; Luciano Burderi ; Tiziana Di Salvo ; Fabrizio Fiore ; Giorgio Matt ; Maria Teresa Menna. Vol. 924 American Institute of Physics, 2007. (AIP Conference Proceedings).

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title = "Secular and orbital changes in emission from J0737-3039 system",

abstract = "The double-pulsar J0737-3039 is not only the most promising system for testing general relativity, but appears a unique laboratory for investigating the so far unaccessible pulsar magnetosphere and the mechanism for radio emission. In fact, the very high orbital inclination gives the possibility of using the radio beams from pulsar A as a probe for investigating the region close to the surface of pulsar B, while relativistic effects modify the system geometry in a timescale suitable for comparing predictions of various models with observation. We present the status of the multi-wavelength observations performed in the 3 years since the discovery and discuss short and long term perspectives for the study of the magnetosphere of pulsar B.",

keywords = "neutron star, pulsar : individual (J0737-3039A, J0737-3039B), DOUBLE PULSAR, RADIO-EMISSION, MODULATION, ECLIPSES",

author = "Andrea Possenti and Marta Burgay and Michael Kramer and Andrew Lyne and Maura McLaughlin and Duncan Lorimer and Ingrid Stairs and Robert Ferdman and Dick Manchester and George Hobbs and Fernando Camilo and Nichi D'Amico and Paulo Freire and John Sarkissian",

year = "2007",

month = aug,

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doi = "10.1063/1.2774915",

language = "English",

isbn = "978-0-7354-0434-2",

volume = "924",

series = "AIP Conference Proceedings",

publisher = "American Institute of Physics",

editor = "Antonelli, {L Angelo} and Israel, {Gian Luca} and Luciano Piersanti and Amedeo Tornambe and Luciano Burderi and {Di Salvo}, Tiziana and Fabrizio Fiore and Giorgio Matt and Menna, {Maria Teresa}",

booktitle = "AIP Conference Proceedings: Multicolored Landscape of Compact Objects and their Explosive Origins",

address = "United States",

note = "Conference on Multicolored Landscape of Compact Objects and Their Explosive Origins ; Conference date: 11-06-2006 Through 18-06-2006",

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Possenti, A, Burgay, M, Kramer, M, Lyne, A, McLaughlin, M, Lorimer, D, Stairs, I, Ferdman, R, Manchester, D, Hobbs, G, Camilo, F, D'Amico, N, Freire, P & Sarkissian, J 2007, Secular and orbital changes in emission from J0737-3039 system. in LA Antonelli, GL Israel, L Piersanti, A Tornambe, L Burderi, T Di Salvo, F Fiore, G Matt & MT Menna (eds), AIP Conference Proceedings: Multicolored Landscape of Compact Objects and their Explosive Origins. vol. 924, AIP Conference Proceedings, vol. 924, American Institute of Physics, Conference on Multicolored Landscape of Compact Objects and Their Explosive Origins, Cefalu, Italy, 11/06/06. https://doi.org/10.1063/1.2774915

Secular and orbital changes in emission from J0737-3039 system. / Possenti, Andrea; Burgay, Marta; Kramer, Michael; Lyne, Andrew; McLaughlin, Maura; Lorimer, Duncan; Stairs, Ingrid; Ferdman, Robert; Manchester, Dick; Hobbs, George; Camilo, Fernando; D'Amico, Nichi; Freire, Paulo; Sarkissian, John.

AIP Conference Proceedings: Multicolored Landscape of Compact Objects and their Explosive Origins. ed. / L Angelo Antonelli; Gian Luca Israel; Luciano Piersanti; Amedeo Tornambe; Luciano Burderi; Tiziana Di Salvo; Fabrizio Fiore; Giorgio Matt; Maria Teresa Menna. Vol. 924 American Institute of Physics, 2007. (AIP Conference Proceedings; Vol. 924).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

TY - GEN

T1 - Secular and orbital changes in emission from J0737-3039 system

AU - Possenti, Andrea

AU - Burgay, Marta

AU - Kramer, Michael

AU - Lyne, Andrew

AU - McLaughlin, Maura

AU - Lorimer, Duncan

AU - Stairs, Ingrid

AU - Ferdman, Robert

AU - Manchester, Dick

AU - Hobbs, George

AU - Camilo, Fernando

AU - D'Amico, Nichi

AU - Freire, Paulo

AU - Sarkissian, John

PY - 2007/8/21

Y1 - 2007/8/21

N2 - The double-pulsar J0737-3039 is not only the most promising system for testing general relativity, but appears a unique laboratory for investigating the so far unaccessible pulsar magnetosphere and the mechanism for radio emission. In fact, the very high orbital inclination gives the possibility of using the radio beams from pulsar A as a probe for investigating the region close to the surface of pulsar B, while relativistic effects modify the system geometry in a timescale suitable for comparing predictions of various models with observation. We present the status of the multi-wavelength observations performed in the 3 years since the discovery and discuss short and long term perspectives for the study of the magnetosphere of pulsar B.

AB - The double-pulsar J0737-3039 is not only the most promising system for testing general relativity, but appears a unique laboratory for investigating the so far unaccessible pulsar magnetosphere and the mechanism for radio emission. In fact, the very high orbital inclination gives the possibility of using the radio beams from pulsar A as a probe for investigating the region close to the surface of pulsar B, while relativistic effects modify the system geometry in a timescale suitable for comparing predictions of various models with observation. We present the status of the multi-wavelength observations performed in the 3 years since the discovery and discuss short and long term perspectives for the study of the magnetosphere of pulsar B.

KW - neutron star

KW - pulsar : individual (J0737-3039A, J0737-3039B)

KW - DOUBLE PULSAR

KW - RADIO-EMISSION

KW - MODULATION

KW - ECLIPSES

U2 - 10.1063/1.2774915

DO - 10.1063/1.2774915

M3 - Conference contribution

SN - 978-0-7354-0434-2

VL - 924

T3 - AIP Conference Proceedings

BT - AIP Conference Proceedings: Multicolored Landscape of Compact Objects and their Explosive Origins

A2 - Antonelli, L Angelo

A2 - Israel, Gian Luca

A2 - Piersanti, Luciano

A2 - Tornambe, Amedeo

A2 - Burderi, Luciano

A2 - Di Salvo, Tiziana

A2 - Fiore, Fabrizio

A2 - Matt, Giorgio

A2 - Menna, Maria Teresa

PB - American Institute of Physics

T2 - Conference on Multicolored Landscape of Compact Objects and Their Explosive Origins

Y2 - 11 June 2006 through 18 June 2006

ER -

Possenti A, Burgay M, Kramer M, Lyne A, McLaughlin M, Lorimer D et al. Secular and orbital changes in emission from J0737-3039 system. In Antonelli LA, Israel GL, Piersanti L, Tornambe A, Burderi L, Di Salvo T, Fiore F, Matt G, Menna MT, editors, AIP Conference Proceedings: Multicolored Landscape of Compact Objects and their Explosive Origins. Vol. 924. American Institute of Physics. 2007. (AIP Conference Proceedings). https://doi.org/10.1063/1.2774915