Skip to main navigation Skip to search Skip to main content

Submillimetre observations of RX J1856.5-3754

  • B. Posselt
  • , K. Schreyer
  • , R. Perna
  • , M. W. Sommer
  • , B. Klein
  • , P. Slane
  • Harvard-Smithsonian Ctr. Astrophys.
  • Astrophysikalisches Institut und Universitäts-Sternwarte Jena
  • University of Bonn
  • Max Planck Institute for Radio Astronomy

Research output: Contribution to journalArticlepeer-review

6 Scopus citations

Abstract

We report on submillimetre bolometer observations of the isolated neutron star RX J1856.5-3754 using the Large Apex Bolometer Camera bolometer array on the Atacama Pathfinder Experiment telescope. No cold dust continuum emission peak at the position of RX J1856.5-3754 was detected. The 3σ flux density upper limit of 5 mJy translates into a cold dust mass limit of a few earth masses. We use the new submillimetre limit, together with a previously obtained H-band limit, to constrain the presence of a gaseous, circumpulsar disc. Adopting a simple irradiated disc model, we obtain a mass accretion limit of and a maximum outer disc radius of ∼1014 cm. By examining the projected proper motion of RX J1856.5-3754, we speculate about a possible encounter of the neutron star with a dense fragment of the CrA molecular cloud a few thousand years ago.

Original languageEnglish
Pages (from-to)1840-1844
Number of pages5
JournalMonthly Notices of the Royal Astronomical Society
Volume405
Issue number3
DOIs
StatePublished - Jul 2010

Keywords

  • Circumstellar matter
  • Stars: individual: RX J1856.5-3754

Fingerprint

Dive into the research topics of 'Submillimetre observations of RX J1856.5-3754'. Together they form a unique fingerprint.

Cite this