Search Publications

Atomic and molecular gas from the epoch of reionisation down to redshift 2
DOI: 10.1051/0004-6361/202142264 Bibcode: 2022A&A...657A..47M

Ciardi, Benedetta; Péroux, Céline; Maio, Umberto

Context. Cosmic gas makes up about 90% of the baryonic matter in the Universe and H2 molecule is the most tightly linked to star formation.
Aims: In this work we study cold neutral gas, its H2 component at different epochs, and corresponding depletion times.
Methods: We perform state-of-the-art hydrodynamic simulati…

2022 Astronomy and Astrophysics
Herschel eHST 21
J-PLUS: Searching for very metal-poor star candidates using the SPEEM pipeline
DOI: 10.1051/0004-6361/202141717 Bibcode: 2022A&A...657A..35G

Sobral, David; Lee, Young Sun; Placco, Vinicius M. +25 more

Context. We explore the stellar content of the Javalambre Photometric Local Universe Survey (J-PLUS) Data Release 2 and show its potential for identifying low-metallicity stars using the Stellar Parameters Estimation based on Ensemble Methods (SPEEM) pipeline.
Aims: SPEEM is a tool used to provide determinations of atmospheric parameters for …

2022 Astronomy and Astrophysics
Gaia 21
Where outflows meet inflows: gas kinematics in SSA22 Ly α blob 2 decoded by advanced radiative transfer modelling
DOI: 10.1093/mnras/stac958 Bibcode: 2022MNRAS.513.3414L

Steidel, Charles C.; Gronke, Max; Li, Zhihui +2 more

We present new spectroscopic observations of Ly α (Ly α) Blob 2 (z ~ 3.1). We observed extended Ly α emission in three distinct regions, where the highest Ly α surface brightness (SB) centre is far away from the known continuum sources. We searched through the MOSFIRE slits that cover the high Ly α SB regions, but were unable to detect any signifi…

2022 Monthly Notices of the Royal Astronomical Society
eHST 21
Expanding Bipolar X-Ray Structure After the 2006 Eruption of RS Oph
DOI: 10.3847/1538-4357/ac4583 Bibcode: 2022ApJ...926..100M

Mukai, K.; Sokoloski, J. L.; Luna, G. J. M. +2 more

We report on the detection and analysis of extended X-ray emission by the Chandra X-ray Observatory stemming from the 2006 eruption of the recurrent nova RS Oph. The extended emission was detected 1254 and 1927 days after the start of the 2006 eruption and is consistent with a bipolar flow oriented in the East-West direction of the sky with openin…

2022 The Astrophysical Journal
Gaia 21
Do AGN triggering mechanisms vary with radio power? - II. The importance of mergers as a function of radio power and optical luminosity
DOI: 10.1093/mnras/stab3231 Bibcode: 2022MNRAS.510.1163P

Tadhunter, C. N.; Ramos Almeida, C.; Pierce, J. C. S. +7 more

Investigation of the triggering mechanisms of radio active galactic nuclei (radio AGN) is important for improving our general understanding of galaxy evolution. In the first paper in this series, detailed morphological analysis of high-excitation radio galaxies (HERGs) with intermediate radio powers suggested that the importance of triggering via …

2022 Monthly Notices of the Royal Astronomical Society
Gaia 21
Successive deuteration in low-mass star-forming regions: The case of D2-methanol (CHD2OH) in IRAS 16293-2422
DOI: 10.1051/0004-6361/202142863 Bibcode: 2022A&A...659A..69D

Margulès, Laurent; Drozdovskaya, Maria N.; Jørgensen, Jes K. +3 more

Context. Di-deuterated molecules are observed in the earliest stages of star formation at abundances of a few percent relative to their nondeuterated isotopologs, which is unexpected considering the scarcity of deuterium in the interstellar medium. With sensitive observations leading to the detection of a steadily increasing number of di-deuterate…

2022 Astronomy and Astrophysics
Rosetta 21
Quasars with Proper Motions and the Link to Double and Multiple AGNs
DOI: 10.3847/1538-4357/ac7047 Bibcode: 2022ApJ...933...28M

Secrest, Nathan J.; Makarov, Valeri V.

Gaia used a large sample of photometrically selected active galactic nuclei (AGNs) and quasars to remove the residual spin of its global proper motion system in order to achieve a maximally inertial reference frame. A small fraction of these reference objects have statistically significant astrometric proper motions in Gaia EDR3. We compile a sour…

2022 The Astrophysical Journal
Gaia 21
A scaled-up planetary system around a supernova progenitor
DOI: 10.1051/0004-6361/202243675 Bibcode: 2022A&A...664A...9S

Quanz, S. P.; Henning, T.; Mayer, L. +24 more

Context. Virtually all known exoplanets reside around stars with M < 2.3 M either due to the rapid evaporation of the protostellar disks or to selection effects impeding detections around more massive stellar hosts.
Aims: To clarify if this dearth of planets is real or a selection effect, we launched the planet-hunting B-star E…

2022 Astronomy and Astrophysics
Gaia 21
The Impact of Energetic Particles on the Martian Ionosphere During a Full Solar Cycle of Radar Observations: Radar Blackouts
DOI: 10.1029/2021JA029535 Bibcode: 2022JGRA..12729535L

Witasse, Olivier; Orosei, Roberto; Lester, Mark +13 more

We present the first long-term characterization of ionization layers in the lower ionosphere of Mars (below ∼90 km), a region inaccessible to orbital in-situ observations, based on an analysis of radar echo blackouts observed on Mars Express and the Mars Reconnaissance Orbiter from 2006 to 2017. A blackout occurs when the expected surface reflecti…

2022 Journal of Geophysical Research (Space Physics)
MEx 21
Mixing Interstellar Clouds Surrounding the Sun
DOI: 10.3847/2041-8213/ac9120 Bibcode: 2022ApJ...937L..32S

Zank, Gary P.; Redfield, Seth; Winslow, Réka M. +9 more

On its journey through the Galaxy, the Sun passes through diverse regions of the interstellar medium. High-resolution spectroscopic measurements of interstellar absorption lines in spectra of nearby stars show absorption components from more than a dozen warm partially ionized clouds within 15 pc of the Sun. The two nearest clouds-the Local Inters…

2022 The Astrophysical Journal
Ulysses 21