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Parkes observations for project P1000 semester 2018OCTS_10

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Parkes observations for project P1000 semester 2018OCTS_10


Hot subdwarf (sdB) stars are core-helium burning stars with thin hydrogen envelopes and masses around 0.5 Msun. A large fraction of sdBs are members of short-period binaries with periods below a few days. Orbital shrinkage through a common envelope phase is the only likely formation channel for such short-period sdB binaries. Although most of th... more


Astronomical and Space Sciences not elsewhere classified


https://doi.org/10.25919/5cbb732f85668


01 Oct 2018


01 Apr 2019


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pulsars neutron stars compact binaries and/or black-holes P1000_2018OCTS


Creative Commons Attribution 4.0 International Licence


CSIRO (Australia)


Kupfer, Thomas; Ravi, Vikram; Geier, Stephan (2018): Parkes observations for project P1000 semester 2018OCTS_10. v1. CSIRO. Data Collection. https://doi.org/10.25919/5cbb732f85668


All Rights (including copyright) CSIRO 2018.


The metadata and files (if any) are available to the public.

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More about this Collection

ivo://au.csiro.atnf/P1000-2018OCTS_10


About this Project

Australia Telescope National Facility


P1000 - A deep search for radio pulsars around hot subdwarf stars in compact binaries


Hot subdwarf stars are core-helium burning stars with thin hydrogen layers. They have masses around half the mass of the sun. Mass transfer with a companion star is required to remove a large fraction of the hydrogen envelope and indeed a large fraction of these objects have a close companion with orbital periods of less than a few days. Most of th... more


Observation


Parkes


Thomas Kupfer


Vikram Ravi


Stephan Geier


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