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91̽»¨
The Cassiopeia A Supernova remnant and its Central Compact Object in X-rays

The Cassiopeia A Supernova remnant and its Central Compact Object as seen by the Chandra X-ray telescope

Credit: NASA/CXC/SAO

Dr. Bettina Posselt

Research Scientist / Affiliate Associate Research Professor (PSU)

Research theme

  • Astronomy and astrophysics

Sub department

  • Astrophysics

Research groups

  • MeerKAT
  • Pulsars, transients and relativistic astrophysics
  • The Square Kilometre Array (SKA)
bettina.posselt@physics.ox.ac.uk
  • About
  • Publications

A Millimeter Continuum Survey for Massive Protoclusters in the Outer Galaxy

The Astrophysical Journal Supplement Series American Astronomical Society 161:2 (2005) 361-393

Authors:

R Klein, B Posselt, K Schreyer, J Forbrich, Th Henning

Direct imaging search for substellar companions around neutron stars

Proceedings of the International Astronomical Union Cambridge University Press (CUP) 1:C200 (2005) 35-40

Authors:

B Posselt, R Neuhäuser, F Haberl

A Millimeter Continuum Survey for Massive Protoclusters in the Outer Galaxy

(2005)

Authors:

R Klein, B Posselt, K Schreyer, J Forbrich, Th Henning

Dense cloud cores in massive star-forming regions

Baltic Astronomy 13:3 (2004) 411-414

Authors:

B Posselt, R Klein, K Schreyer, T Henning

Abstract:

We have performed a submillimeter survey of the areas around 47 selected IRAS point sources of high luminosity. A number of new submm sources were found. The high multiplicity of the sources suggests that isolated massive-star formation is a rare event. In some cases the filaments near the young stellar objects (YSO) or between them were found. The pointers of massive star formation like masers, outflows and high-density knots were identified. Available catalogs in the near-infrared (2MASS), mid-infrared (MSX point sources) and radio continuum (NVSS at 1.4 GHz point sources) were correlated to our submm maps.

An Extremely Young Massive Stellar Object near IRAS 07029–1215

The Astrophysical Journal American Astronomical Society 602:2 (2004) 843-849

Authors:

J Forbrich, K Schreyer, B Posselt, R Klein, Th Henning

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