Macquarie University, Sydney Macquarie University ResearchOnline

Showing items 1 - 5 of 5.

Add to Quick Collection   All 5 Results

  • First
  • Previous
  • 1
  • Next
  • Last
Sort:
 Add All Items to Quick Collection
Authors: Douchin, Dimitri
Date: 2015
Language: eng
Resource Type: Thesis PhD
Identifier: http://hdl.handle.net/1959.14/1068333
Description: "A PhD thesis submitted to Macquarie University in cotutelle with Université de Montpellier 2 Department of Physics and Astronomy January 2015"
Full Text: Full Text
Date: 2015
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/362826
Description: There is no conclusive explanation of why ∼80 per cent of planetary nebulae (PNe) are non-spherical. In the Binary Hypothesis, a binary interaction is a preferred channel to form a non-spherical PN. A ... More
Reviewed: Reviewed
Date: 2013
Language: eng
Resource Type: journal article
Identifier: http://hdl.handle.net/1959.14/271336
Description: A measurement by microlensing of the planetary mass function of planets with masses ranging from 5 M⊕ to 10 MJ and orbital radii from 0.5 to 10 au was reported recently. A strategy for extending the m ... More
Reviewed: Reviewed
Date: 2012
Subject Keyword: planetary nebulae: general | surveys
Language: eng
Resource Type: conference paper
Identifier: http://hdl.handle.net/1959.14/216121
Description: Having surveyed ≈ 10% of the sky, we have identified more than 130 PN candidates by surveying multicolour Digitized Sky Survey (DSS), Sloan Digitized Sky Survey (SDSS), and combined [O III], Hα and [S ... More
Full Text: Full Text
Date: 2012
Language: eng
Resource Type: conference paper
Identifier: http://hdl.handle.net/1959.14/208223
Description: The Kepler Observatory offers unprecedented photometric precision (<1 mmag) and cadence for monitoring the central stars of planetary nebulae, allowing the detection of tiny periodic light curve varia ... More
  • First
  • Previous
  • 1
  • Next
  • Last