Hamish Barker
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View article: Spectral evolution of the narrow emission line components in optical during the 2022 nova eruption of U Scorpii
Spectral evolution of the narrow emission line components in optical during the 2022 nova eruption of U Scorpii Open
There remains debate over whether the accretion disk survives or is entirely disrupted after the nova eruption. In our previous paper, Muraoka et al. (2024, PASJ, 76, 293) have photometrically demonstrated that the surviving accretion disk…
View article: Author Correction: A planetary collision afterglow and transit of the resultant debris cloud
Author Correction: A planetary collision afterglow and transit of the resultant debris cloud Open
View article: A planetary collision afterglow and transit of the resultant debris cloud
A planetary collision afterglow and transit of the resultant debris cloud Open
Planets grow in rotating disks of dust and gas around forming stars, some of which can subsequently collide in giant impacts after the gas component is removed from the disk. Monitoring programs with the warm Spitzer mission have recorded …
View article: A planetary collision afterglow and transit of the resultant debris cloud
A planetary collision afterglow and transit of the resultant debris cloud Open
View article: ASASSN-21qj astronomical observations
ASASSN-21qj astronomical observations Open
Data from astronomical observatories looking at the star ASASSN-21qj.
View article: ASASSN-21qj astronomical observations
ASASSN-21qj astronomical observations Open
Data from astronomical observatories looking at the star ASASSN-21qj.
View article: V618 Sgr: Galactic eclipsing symbiotic nova detected in repeated outbursts
V618 Sgr: Galactic eclipsing symbiotic nova detected in repeated outbursts Open
V618 Sgr was previously classified as an R CrB-type variable and later as a possible symbiotic star. Our study aims to analyse the nature of this target, which is currently undergoing significant brightening in properties similar to those …
View article: Gaia22eor: Symbiotic Star V2756 Sgr Detected in a Deep Eclipse
Gaia22eor: Symbiotic Star V2756 Sgr Detected in a Deep Eclipse Open
V2756 Sgr is a long-known S-type symbiotic binary that was recently detected in ∼1 mag eclipse-like fading by the Gaia satellite. This behavior was reported as a Gaia Science Alert under the designation Gaia22eor. V2756 Sgr has not been re…
View article: ASASSN-21co: A Detached Eclipsing Binary with an 11.9 yr Period
ASASSN-21co: A Detached Eclipsing Binary with an 11.9 yr Period Open
We use ASAS V -band and ASAS-SN g -band observations to model the long-period detached eclipsing binary ASASSN-21co. ASAS observations show an eclipse of depth V ∼ 0.6 mag in 2009 April. ASAS-SN g -band observations from 2021 March show an…