431 research outputs found
The enigmatic central star of the planetary nebula PRTM 1
The central star of the planetary nebula PRTM 1 (PN G243.8-37.1) was
previously found to be variable by M. Pena and colleagues. As part of a larger
programme aimed towards finding post common-envelope binary central stars we
have monitored the central star of PRTM 1 spectroscopically and photometrically
for signs of variability. Over a period of ~3 months we find minimal radial
velocity (<10 km/s) and photometric (< 0.2 mag) variability. The data suggest a
close binary nucleus can be ruled out at all but the lowest orbital
inclinations, especially considering the spherical morphology of the nebula
which we reveal for the first time. Although the current data strongly support
the single star hypothesis, the true nature of the central star of PRTM 1
remains enigmatic and will require further radial velocity monitoring at higher
resolution to rule out a close binary. If in the odd case that it is a close
binary, it would be the first such case in a spherical planetary nebula, in
contradiction to current thinking.Comment: A&A, in pres
Ongoing surveys for close binary central stars and wider implications
Binary central stars have long been invoked to explain the vexing shapes of
planetary nebulae (PNe) despite there being scant direct evidence to support
this hypothesis. Modern large-scale surveys and improved observing strategies
have allowed us to significantly boost the number of known close binary central
stars and estimate at least 20% of PNe have close binary nuclei that passed
through a common-envelope (CE) phase. The larger sample of post-CE nebulae
appears to have a high proportion of bipolar nebulae, low-ionisation structures
(especially in SN1987A-like rings) and polar outflows or jets. These trends are
guiding our target selection in ongoing multi-epoch spectroscopic and
photometric surveys for new binaries. Multiple new discoveries are being
uncovered that further strengthen the connection between post-CE trends and
close binaries. These ongoing surveys also have wider implications for
understanding CE evolution, low-ionisation structure and jet formation,
spectral classification of central stars, asymptotic giant branch (AGB)
nucleosynthesis and dust obscuration events in PNe.Comment: To appear in IAU Symposium 283: Planetary Nebulae, an Eye to the
Future. 4 pages, 1 figur
- …