Click here to view this collection in the new DAP user interface
Parkes observations for project P1014 semester 2019OCTS_03
The spatial distribution of neutral gas is important for understanding the interstellar medium (ISM) evolution and star formation. However, the distribution of Tiny Scale Atomic Structures (TSAS), especially the extremely small scale structures with spatial scales ranging from a few to hundreds of AU are largely unexplored. The formation and evolut... moreion of TSAS are still on an active debate. Multi-epoch observations of HI absorption against pulsars are a tested, practical observational method to probe the TSAS, due to pulsar’s nature on-off state and proper motions of 1 to 100 AU per year. We thus propose two epoch observations, which are separated by about five months, for three bright pulsars for probing structures ranging from 8 to 1900 AU. less
Astronomical and Space Sciences not elsewhere classified
01 Oct 2019
31 Mar 2020
interstellar medium in and around the Milky Way
Creative Commons Attribution 4.0 International Licence
Liu, Mengting; Dawson, Joanne; Hobbs, George; Stanimirovic, Snezana; Li, Di; Krco, Marko (2019): Parkes observations for project P1014 semester 2019OCTS_03. v1. CSIRO. Data Collection.
All Rights (including copyright) CSIRO 2019.
Access to this collection's metadata and/or files (if any) are restricted until 30 Sep 2021.
Australia Telescope National Facility
P1014 - A Search For Small Scale Structures in the ISM (Few to Hundreds of AU Scales) Using the new Parkes UWL Receiver
Pulsars are a quickly rotating neutron star with a regular rotation period traveling through the interstellar medium with velocities of a few to hundreds of kilometers per second. Observations towards pulsars at different time epochs using the new Parkes UWL receiver with multiple spectral windows will probe tiny scale structures and detect the int... moreerstellar molecules in them. This observation will help us to understand the distribution and evolution of tiny scale structures in our galaxy leading to a better understanding of the dissipative processes in the ISM during star formation less