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Absolute V-band magnitudes and mass-to-light ratios of Galactic globular clusters
DOI: 10.1017/pasa.2020.38 Bibcode: 2020PASA...37...46B

Hilker, M.; Baumgardt, H.; Sollima, A.

We have used Hubble Space Telescope and ground-based photometry to determine total V-band magnitudes and mass-to-light ratios of more than 150 Galactic globular clusters. We do this by summing up the magnitudes of their individual member stars, using colour-magnitude information, Gaia DR2 proper motions, and radial velocities to distinguish cluste…

2020 Publications of the Astronomical Society of Australia
Gaia eHST 54
Galaxy spin direction distribution in HST and SDSS show similar large-scale asymmetry
DOI: 10.1017/pasa.2020.46 Bibcode: 2020PASA...37...53S

Shamir, Lior

Several recent observations using large data sets of galaxies showed non-random distribution of the spin directions of spiral galaxies, even when the galaxies are too far from each other to have gravitational interaction. Here, a data set of$\sim8.7\cdot10^3$spiral galaxies imaged byHubble Space Telescope(HST) is used to test and profile a possibl…

2020 Publications of the Astronomical Society of Australia
eHST 18
A SETI survey of the Vela region using the Murchison Widefield Array: Orders of magnitude expansion in search space
DOI: 10.1017/pasa.2020.27 Bibcode: 2020PASA...37...35T

Tremblay, C. D.; Tingay, S. J.

Following the results of our previous low-frequency searches for extraterrestrial intelligence (SETI) using the Murchison Widefield Array (MWA), directed towards the Galactic Centre and the Orion Molecular Cloud (Galactic Anticentre), we report a new large-scale survey towards the Vela region with the lowest upper limits thus far obtained with the…

2020 Publications of the Astronomical Society of Australia
Gaia 15
PKS 2250-351: A giant radio galaxy in Abell 3936
DOI: 10.1017/pasa.2019.49 Bibcode: 2020PASA...37...13S

Seymour, N.; Leahy, D. A.; Norris, R. P. +27 more

We present a detailed analysis of the radio galaxy PKS $2250{-}351$ , a giant of 1.2 Mpc projected size, its host galaxy, and its environment. We use radio data from the Murchison Widefield Array, the upgraded Giant Metre-wavelength Radio Telescope, the Australian Square Kilometre Array Pathfinder, and the Australia Telescope Compact Array to mode…

2020 Publications of the Astronomical Society of Australia
Herschel 14
ASKAP reveals giant radio halos in two merging SPT galaxy clusters
DOI: 10.1017/pasa.2020.34 Bibcode: 2020PASA...37...40W

Johnston-Hollitt, Melanie; Akamatsu, Hiroki; Hodgson, Torrance +4 more

Early science observations from the Australian Square Kilometre Array Pathfinder (ASKAP) have revealed clear signals of diffuse radio emission associated with two clusters detected by the South Pole Telescope via their Sunyaev Zel'dovich signal: SPT CLJ0553-3342 (MACS J0553.4-3342) and SPT CLJ0638-5358 (Abell S0592) are both high-mass lensing clus…

2020 Publications of the Astronomical Society of Australia
eHST 14
Investigation on the mass transferring near-contact binary TT Cet
DOI: 10.1017/pasa.2020.22 Bibcode: 2020PASA...37...31T

Tian, Xiao-Man; Chang, Lin-Feng

First multi-colour complete light curves and low-resolution spectra of short-period eclipsing binary TT Cet are presented. The stellar atmospheric parameters of the primary star were derived through spectra fitting as: $T_{eff}=7 091±124 {K}$, $\log g = 4.15±0.33 {cm}/s^2$, and $[Fe/H]=-0.23±0.04 dex$. The light curves were analysed using the Wils…

2020 Publications of the Astronomical Society of Australia
Gaia 6
The stellar rotation-activity relation for a sample of SuperWASP and ASAS-SN field stars
DOI: 10.1017/pasa.2020.33 Bibcode: 2020PASA...37...42T

Thiemann, Heidi B.; Norton, Andrew J.; Kolb, Ulrich C.

It is well established that late-type main-sequence (MS) stars display a relationship between X-ray activity and the Rossby number, Ro, the ratio of rotation period to the convective turnover time. This manifests itself as a saturated regime (where X-ray activity is constant) and an unsaturated regime (where X-ray activity anti-correlates with Ros…

2020 Publications of the Astronomical Society of Australia
Gaia XMM-Newton 4
A hundred new eclipsing binary system candidates studied in a near-infrared window in the VVV survey
DOI: 10.1017/pasa.2020.44 Bibcode: 2020PASA...37...54G

Minniti, D.; Saito, R. K.; Palma, T. +4 more

We present the first results obtained from an extensive study of eclipsing binary (EB) system candidates recently detected in the VISTA Variables in the Vía Láctea (VVV) near-infrared (NIR) Survey. We analyse the VVV tile d040 in the southern part of the Galactic disc wherein the interstellar reddening is comparatively low, which makes it possible…

2020 Publications of the Astronomical Society of Australia
Gaia 4
Investigation of the coronal heating through phase relation of solar activity indexes
DOI: 10.1017/pasa.2019.43 Bibcode: 2020PASA...37....1L

Li, K. J.; Xu, J. C.; Yin, Z. Q. +2 more

The coronal heating problem is a long-standing perplexing issue. In this study, 13 solar activity indexes are used to investigate their phase relation with the sunspot number (SSN). Only three of them are found to statistically significantly lag the SSN (large-scale magnetic activity) by about one solar rotation period; the three indexes are total…

2020 Publications of the Astronomical Society of Australia
SOHO 4
Bridging the ultraviolet and optical regions: Transformation equations between GALEX and UBV photometric systems
DOI: 10.1017/pasa.2020.12 Bibcode: 2020PASA...37...22B

Bilir, S.; Ak, T.; Yontan, T. +6 more

We derive transformation equations between GALEX and UBV colours by using the reliable data of 556 stars. We present two sets of equations: as a function of (only) luminosity class and as a function of both luminosity class and metallicity. The metallicities are provided from the literature, while the luminosity classes are determined by using the…

2020 Publications of the Astronomical Society of Australia
Gaia 3