Greaves, Jane and Holland, W. S. 2017. The Geminga pulsar wind nebula in the mid-infrared and submillimetre. Monthly Notices of the Royal Astronomical Society: Letters 471 (1) , L26-L30. 10.1093/mnrasl/slx098 |
|
PDF
- Published Version
Available under License Creative Commons Attribution No Derivatives. Download (600kB) | Preview |
Abstract
The nearby middle-aged Geminga pulsar has crossed the Galactic plane within the last ∼0.1 Myr. We present archival data from Wide-field Infrared Survey Explorer and from SCUBA and SCUBA-2 on the James Clerk Maxwell Telescope to assess whether any midinfrared and submillimetre emission arises from interaction of the pulsar wind nebula with the interstellar medium. A candidate shell and bow shock are reported. Given the low pulsar velocity and local density, dust grains appear able to penetrate into the nebula. A compact source seen towards the pulsar is fitted with a dust spectrum. If confirmed as a real association at higher resolution, this could be a circum-pulsar disc of at least a few Earth-masses, in which future planets could form.
Item Type: | Article |
---|---|
Date Type: | Publication |
Status: | Published |
Schools: | Physics and Astronomy |
Subjects: | Q Science > QB Astronomy |
Publisher: | Oxford University Press |
ISSN: | 17453925 |
Date of First Compliant Deposit: | 9 November 2017 |
Date of Acceptance: | 13 June 2017 |
Last Modified: | 09 Nov 2017 15:47 |
URI: | http://orca.cf.ac.uk/id/eprint/106381 |
Actions (repository staff only)
![]() |
Edit Item |