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Imprints of Neutron Stars in the Interstellar Medium

Published online by Cambridge University Press:  19 July 2016

Estela M. Reynoso ,
Simon Johnston ,
Anne J. Green ,
W. M. Goss ,
Gloria M. Dubner  and
Elsa B. Giacani
Estela M. Reynoso
Affiliation:
Instituto de Astronomía y Física del Espacio (IAFE), c.c. 67, Suc. 28, 1428 Buenos Aires, Argentina School of Physics A29, University of Sydney, NSW 2006, Australia
Simon Johnston
Affiliation:
School of Physics A29, University of Sydney, NSW 2006, Australia
Anne J. Green
Affiliation:
School of Physics A29, University of Sydney, NSW 2006, Australia
W. M. Goss
Affiliation:
National Radio Astronomy Observatory, PO Box O, Socorro, NM 87801, USA
Gloria M. Dubner
Affiliation:
IAFE, c.c. 67, Suc. 28, 1428 Buenos Aires, Argentina
Elsa B. Giacani
Affiliation:
IAFE, c.c. 67, Suc. 28, 1428 Buenos Aires, Argentina

Abstract

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We have carried out an H I survey towards X-ray central compact objects (CCOs) inside supernova remnants (SNRs), which shows that many of them are placed within local H I minimA. The nature of these minima is not clear, but the most likely explanation is that the CCOs have evacuated the neighboring gas. This survey also allowed us to detect a weak, diffuse radio nebula inside the SNR G266.2−1.2, probably created by the winds of its associated CCO.

Type
Part 5: Magnetars, Central Compact Objects and Isolated Neutron Stars
Information
Symposium - International Astronomical Union , Volume 218: Young Neutrons Stars and their Environments , 2004 , pp. 277 - 278
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

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