Search Publications

The Ionizing Spectra of Extremely Metal-poor O Stars: Constraints from the Only H II Region in Leo P
DOI: 10.3847/1538-4357/aca896 Bibcode: 2023ApJ...943...65T

McQuinn, Kristen B. W.; Chisholm, John; Berg, Danielle A. +1 more

Metal-poor, star-forming dwarf galaxies produce extreme nebular emission and likely played a major role in cosmic reionization. Yet, determining their contribution to the high-redshift ionizing photon budget is hampered by the lack of observations constraining the ionizing spectra of individual massive stars more metal-poor than the Magellanic Clo…

2023 The Astrophysical Journal
eHST 18
Evidence of extended cold molecular gas and dust haloes around z ∼ 2.3 extremely red quasars with ALMA
DOI: 10.1093/mnras/stac3787 Bibcode: 2023MNRAS.519.5246S

Maiolino, R.; Carniani, S.; Scholtz, J. +1 more

Large-scale outflows are believed to be an important mechanism in the evolution of galaxies. We can determine the impact of these outflows by studying either current galaxy outflows and their effect in the galaxy or by studying the effect of past outflows on the gas surrounding the galaxy. In this work, we examine the CO(7-6), [C I] ($^{3} \rm P_{…

2023 Monthly Notices of the Royal Astronomical Society
eHST 18
The geometric albedo of the hot Jupiter HD 189733b measured with CHEOPS
DOI: 10.1051/0004-6361/202245016 Bibcode: 2023A&A...672A..24K

Guterman, P.; Alonso, R.; Deleuil, M. +84 more

Context. Measurements of the occultation of an exoplanet at visible wavelengths allow us to determine the reflective properties of a planetary atmosphere. The observed occultation depth can be translated into a geometric albedo. This in turn aids in characterising the structure and composition of an atmosphere by providing additional information o…

2023 Astronomy and Astrophysics
CHEOPS eHST 18
On the Evolution of the Anisotropic Scaling of Magnetohydrodynamic Turbulence in the Inner Heliosphere
DOI: 10.3847/1538-4357/acc658 Bibcode: 2023ApJ...951..141S

Horbury, T. S.; Velli, Marco; Dudok de Wit, Thierry +20 more

We analyze a merged Parker Solar Probe (PSP) and Solar Orbiter (SO) data set covering heliocentric distances 13 R ≲ R ≲ 220 R to investigate the radial evolution of power and spectral index anisotropy in the wavevector space of solar wind turbulence. Our results show that anisotropic signatures of turbulence display a dis…

2023 The Astrophysical Journal
SolarOrbiter 18
A three-component giant radio halo: The puzzling case of the galaxy cluster Abell 2142
DOI: 10.1051/0004-6361/202347245 Bibcode: 2023A&A...678A.133B

Brunetti, G.; Rossetti, M.; De Grandi, S. +16 more

Context. Turbulence introduced into the intracluster medium (ICM) through cluster-merger events transfers energy to non-thermal components, and can trigger the formation of diffuse synchrotron radio sources. Typical diffuse sources in the form of giant radio halos and mini-halos are found in merging and relaxed cool-core galaxy clusters, respectiv…

2023 Astronomy and Astrophysics
XMM-Newton 18
ESCARGOT: Mapping Vertical Phase Spiral Characteristics Throughout the Real and Simulated Milky Way
DOI: 10.3847/1538-4357/acf1fc Bibcode: 2023ApJ...955...74D

Price-Whelan, Adrian M.; Johnston, Kathryn V.; Darragh-Ford, Elise +1 more

The recent discovery of a spiral pattern in the vertical kinematic structure in the solar neighborhood provides a prime opportunity to study nonequilibrium dynamics in the Milky Way from local stellar kinematics. Furthermore, results from simulations indicate that even in a limited volume, differences in stellar orbital histories allow us to trace…

2023 The Astrophysical Journal
Gaia 18
The extremely high albedo of LTT 9779 b revealed by CHEOPS. An ultrahot Neptune with a highly metallic atmosphere
DOI: 10.1051/0004-6361/202346117 Bibcode: 2023A&A...675A..81H

Deleuil, M.; Scandariato, G.; Hoyer, S. +11 more

Context. Optical secondary eclipse measurements of small planets can provide a wealth of information about the reflective properties of these worlds, but the measurements are particularly challenging to attain because of their relatively shallow depth. If such signals can be detected and modeled, however, they can provide planetary albedos, therma…

2023 Astronomy and Astrophysics
CHEOPS Gaia 18
A Survey for High-redshift Gravitationally Lensed Quasars and Close Quasar Pairs. I. The Discoveries of an Intermediately Lensed Quasar and a Kiloparsec-scale Quasar Pair at z 5
DOI: 10.3847/1538-3881/acc2be Bibcode: 2023AJ....165..191Y

Fan, Xiaohui; Yang, Jinyi; Wang, Feige +1 more

We present the first results from a new survey for high-redshift (z ≳ 5) gravitationally lensed quasars and close quasar pairs. We carry out candidate selection based on the colors and shapes of objects in public imaging surveys, then conduct follow-up observations to confirm the nature of high-priority candidates. In this paper, we report the dis…

2023 The Astronomical Journal
Gaia eHST 18
First results from the Solar Orbiter Heavy Ion Sensor
DOI: 10.1051/0004-6361/202346304 Bibcode: 2023A&A...676A..36L

Fedorov, A.; Livi, S.; Wurz, P. +30 more


Aims: Solar Orbiter launched in February 2020 with the goal of revealing the connections between the Sun's interior, atmosphere, and the heliosphere. The Solar Orbiter Heavy Ion Sensor (HIS) is a time-of-flight ion mass spectrometer dedicated to measuring heavy ions in the solar wind.
Methods: We present an overview of the first measurem…

2023 Astronomy and Astrophysics
SolarOrbiter 18
Protoplanetary disks in Ks-band total intensity and polarized light
DOI: 10.1051/0004-6361/202347353 Bibcode: 2023A&A...680A.114R

Ren, Bin B.; Ménard, François; Bae, Jaehan +11 more

Context. The diverse morphology among protoplanetary disks may result from planet-disk interactions, suggesting the presence of planets undergoing formation. The characterization of disks can provide information on the formation environments of planets. To date, most imaging campaigns have probed the polarized light from disks, which is only a fra…

2023 Astronomy and Astrophysics
Gaia 18