Search Publications

Distances, extinctions, and stellar parameters for stars in SkyMapper DR3
DOI: 10.1093/mnras/stab3326 Bibcode: 2022MNRAS.510..433L

Lin, Jane; Casagrande, Luca; Asplund, Martin

We present a Bayesian isochrone fitting machinery to derive distances, extinctions, and stellar parameters (Teff, log g, and $\rm [Fe/H]$) for stars in the SkyMapper data release 3 (DR3) survey. We complement the latter with photometry from Gaia, 2MASS, and AllWISE, in addition to priors on parallaxes and interstellar extinction. We fin…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 5
Quantification of O2 formation during UV photolysis of water ice: H2O and H2O:CO2 ices
DOI: 10.1051/0004-6361/202141875 Bibcode: 2022A&A...657A.120B

Linnartz, H.; Chuang, K. -J.; Fedoseev, G. +4 more

Context. The Rosetta and Giotto missions investigated the composition of the cometary comae of 67P/Churyumov-Gerasimenko and 1P/Halley, respectively. In both cases, a surprisingly large amount of molecular oxygen (O2) was detected and was well correlated with the observed abundances of H2O. Laboratory experiments simulating c…

2022 Astronomy and Astrophysics
Rosetta 5
Development of a cometosheath at comet 67P/Churyumov-Gerasimenko. A case study comparison of Rosetta observations
DOI: 10.1051/0004-6361/202142461 Bibcode: 2022A&A...660A.103W

Nilsson, H.; Goetz, C.; Stenberg Wieser, G. +2 more

Context. The ionosphere of a comet is known to deflect the solar wind through mass loading, but the interaction is dependent on cometary activity. We investigate the details of this process at comet 67P using the Rosetta Ion Composition Analyzer.
Aims: This study aims to compare the interaction of the solar wind and cometary ions during two d…

2022 Astronomy and Astrophysics
Rosetta 5
The SDSS-Gaia View of the Color-Magnitude Relation for Blue Horizontal-branch Stars
DOI: 10.3847/1538-4357/ac983f Bibcode: 2022ApJ...940...30B

Limberg, Guilherme; Rossi, Silvia; Perottoni, Hélio D. +3 more

We present an updated sample of blue horizontal-branch (BHB) stars selected from the photometric and spectroscopic data from Sloan Digital Sky Survey and its associated project Sloan Extension for Galactic Understanding and Exploration (SEGUE). With these data, we selected candidates for A-type stars in the color-color space and then a mixture mod…

2022 The Astrophysical Journal
Gaia 5
Winter Weakening of Titan's Stratospheric Polar Vortices
DOI: 10.3847/PSJ/ac5ea1 Bibcode: 2022PSJ.....3...73S

Toigo, A. D.; Teanby, N. A.; Newman, C. E. +3 more

Polar vortices are a prominent feature in Titan's stratosphere. The Cassini mission has provided a detailed view of the breakdown of the northern polar vortex and formation of the southern vortex, but the mission did not observe the full annual cycle of the evolution of the vortices. Here we use a TitanWRF general circulation model simulation of a…

2022 The Planetary Science Journal
Cassini 5
A multi-instrument investigation of the frequency stability of oscillations above the acoustic cut-off frequency with solar activity
DOI: 10.1093/mnras/stac647 Bibcode: 2022MNRAS.512.5743K

Broomhall, A. -M.; Kiefer, R.; Kosak, K.

Below the acoustic cut-off frequency, oscillations are trapped within the solar interior and become resonant. However, signatures of oscillations persist above the acoustic cut-off frequency, and these travelling waves are known as pseudo-modes. Acoustic oscillation frequencies are known to be correlated with the solar cycle, but the pseudo-mode f…

2022 Monthly Notices of the Royal Astronomical Society
SOHO 5
IGR J18249-3243: a new GeV-emitting FR II and the emerging population of high-energy radio galaxies
DOI: 10.1093/mnras/stac865 Bibcode: 2022MNRAS.513..886B

Ricci, R.; Wieringa, M. H.; Giroletti, M. +10 more

The advent of new all-sky radio surveys such as the VLA Sky Survey and the Rapid ASKAP Continuum Survey, performed with the latest generation radio telescopes, is opening new possibilities on the classification and study of extragalactic γ-ray sources, specially the underrepresented ones like radio galaxies. In particular, the enhanced sensitivity…

2022 Monthly Notices of the Royal Astronomical Society
INTEGRAL XMM-Newton 5
A 3D Physics-Based Particle Model of the Venus Oxygen Corona: Variations With Solar Activity
DOI: 10.1029/2021JA030168 Bibcode: 2022JGRA..12730168T

Combi, Michael R.; Tenishev, Valeriy; Shou, Yinsi +2 more

Due to Venus not having a substantial planetary magnetic field the fast-flowing solar wind plasma can propagate to regions close to the planet. Therefore, thermal atomic oxygen in the thermosphere, hot oxygen in the corona, and the resulting pickup oxygen ions are essential for determining the overall interaction of the planet with plasma of the a…

2022 Journal of Geophysical Research (Space Physics)
VenusExpress 5
Ultraviolet spectropolarimetry with Polstar: using Polstar to test magnetospheric mass-loss quenching
DOI: 10.1007/s10509-022-04113-x Bibcode: 2022Ap&SS.367..120S

Cheung, M. C. M.; Wade, G. A.; Nazé, Y. +17 more

Polstar is a proposed NASA MIDEX space telescope that will provide high-resolution, simultaneous full-Stokes spectropolarimetry in the far ultraviolet, together with low-resolution linear polarimetry in the near ultraviolet. This observatory offers unprecedented capabilities to obtain unique information on the magnetic and plasma properties of the…

2022 Astrophysics and Space Science
IUE 5
Hard X-Ray Flares and Spectral Variability in NGC 4395 ULX1
DOI: 10.3847/1538-4357/ac8f8f Bibcode: 2022ApJ...938...76G

Bachetti, Matteo; Rana, Vikram; Ghosh, Tanuman

We report the detection of flaring events in NGC 4395 ULX1, a nearby ultraluminous X-ray source (ULX), for the first time, using recent XMM-Newton observations. The flaring episodes are spectrally harder than the steady-emission intervals, resulting in higher fractional variability in the high-energy regime. A thin Keplerian and a slim accretion d…

2022 The Astrophysical Journal
XMM-Newton 5