Search Publications

Charting nearby dust clouds using Gaia data only
DOI: 10.1051/0004-6361/201935093 Bibcode: 2019A&A...631A..32L

Enßlin, T. A.; Leike, R. H.


Aims: Highly resolved maps of the local Galactic dust are an important ingredient for sky emission models. Over almost the whole electromagnetic spectrum one can see imprints of dust, many of which originate from dust clouds within 300 pc. Having a detailed 3D reconstruction of these local dust clouds enables detailed studies, helps to quanti…

2019 Astronomy and Astrophysics
Gaia 61
Multi-wavelength Properties of Type 1 and Type 2 AGN Host Galaxies in the Chandra-COSMOS Legacy Survey
DOI: 10.3847/1538-4357/ab01fb Bibcode: 2019ApJ...872..168S

Lusso, Elisabeta; Marchesi, Stefano; Onodera, Masato +6 more

We investigate the multi-wavelength properties of host galaxies of 3701 X-ray-selected active galactic nuclei (AGNs) out to z ∼ 5 in the Chandra-COSMOS Legacy Survey. Thanks to the extensive multi-wavelength photometry available in the COSMOS field, we derive AGN luminosities, host stellar masses, and star formation rates (SFRs) via a multi-compon…

2019 The Astrophysical Journal
Herschel 61
Dissecting the AGN Disk-Jet System with Joint VLBI-Gaia Analysis
DOI: 10.3847/1538-4357/aaf650 Bibcode: 2019ApJ...871..143P

Kovalev, Y. Y.; Plavin, A. V.; Petrov, L. Y.

We analyze differences in positions of active galactic nuclei (AGNs) between Gaia data release 2 and very long baseline interferometry (VLBI) and compare the significant VLBI-to-Gaia offsets in more than 1000 objects with their jet directions. Remarkably at least three-fourths of the significant offsets are confirmed to occur downstream or upstrea…

2019 The Astrophysical Journal
Gaia 61
Barium and related stars, and their white-dwarf companions. II. Main-sequence and subgiant starss
DOI: 10.1051/0004-6361/201935390 Bibcode: 2019A&A...626A.128E

Jorissen, A.; Pourbaix, D.; Escorza, A. +12 more

Barium (Ba) dwarfs and CH subgiants are the less evolved analogues of Ba and CH giants. They are F- to G-type main-sequence stars polluted with heavy elements by their binary companions when the companion was on the asymptotic giant branch (AGB). This companion is now a white dwarf that in most cases cannot be directly detected. We present a large…

2019 Astronomy and Astrophysics
Gaia Hipparcos 61
ALMA captures feeding and feedback from the active galactic nucleus in NGC 613
DOI: 10.1051/0004-6361/201935845 Bibcode: 2019A&A...632A..33A

Krips, M.; van der Werf, P.; Combes, F. +11 more

We report ALMA observations of CO(3-2) emission in the Seyfert/nuclear starburst galaxy NGC 613, at a spatial resolution of 17 pc, as part of our NUclei of GAlaxies (NUGA) sample. Our aim is to investigate the morphology and dynamics of the gas inside the central kiloparsec, and to probe nuclear fueling and feedback phenomena. The morphology of CO…

2019 Astronomy and Astrophysics
eHST 61
Probing the existence of very massive first stars
DOI: 10.1093/mnras/stz1464 Bibcode: 2019MNRAS.487.4261S

Salvadori, S.; Bonifacio, P.; Caffau, E. +4 more

We present a novel approach aimed at identifying the key chemical elements to search for the (missing) descendants of very massive first stars exploding as pair instability supernovae (PISN). Our simple and general method consists in a parametric study accounting for the unknowns related to early cosmic star formation and metal-enrichment. Our app…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 61
Reference Star Differential Imaging of Close-in Companions and Circumstellar Disks with the NIRC2 Vortex Coronagraph at the W. M. Keck Observatory
DOI: 10.3847/1538-3881/aafee2 Bibcode: 2019AJ....157..118R

Matthews, Keith; Serabyn, Eugene; Absil, Olivier +11 more

Reference star differential imaging (RDI) is a powerful strategy for high-contrast imaging. Using example observations taken with the vortex coronagraph mode of Keck/NIRC2 in L‧ band, we demonstrate that RDI provides improved sensitivity to point sources at small angular separations compared to angular differential imaging (ADI). Applying RDI to i…

2019 The Astronomical Journal
Gaia Hipparcos 60
Revisiting long-standing puzzles of the Milky Way: the Sun and its vicinity as typical outer disk chemical evolution
DOI: 10.1051/0004-6361/201834155 Bibcode: 2019A&A...625A.105H

Haywood, M.; Lehnert, M. D.; Di Matteo, P. +2 more

We present a scenario of the chemical enrichment of the solar neighborhood that solves the G-dwarf problem by taking into account constraints on a larger scale. We argue that the Milky Way disk within 10 kpc has been enriched to solar metallicity by a massive stellar population: the thick disk, which itself formed from a massive turbulent gaseous …

2019 Astronomy and Astrophysics
Gaia 60
Independent confirmation of a methane spike on Mars and a source region east of Gale Crater
DOI: 10.1038/s41561-019-0331-9 Bibcode: 2019NatGe..12..326G

Cardesín-Moinelo, Alejandro; Marín-Yaseli de la Parra, Julia; Aoki, Shohei +11 more

Reports of methane detection in the Martian atmosphere have been intensely debated. The presence of methane could enhance habitability and may even be a signature of life. However, no detection has been confirmed with independent measurements. Here, we report a firm detection of 15.5 ± 2.5 ppb by volume of methane in the Martian atmosphere above G…

2019 Nature Geoscience
MEx 60
The tidal disruption event AT2017eqx: spectroscopic evolution from hydrogen rich to poor suggests an atmosphere and outflow
DOI: 10.1093/mnras/stz1837 Bibcode: 2019MNRAS.488.1878N

Berger, E.; Challis, P.; Foley, R. J. +24 more

We present and analyse a new tidal disruption event (TDE), AT2017eqx at redshift z = 0.1089, discovered by Pan-STARRS and ATLAS. The position of the transient is consistent with the nucleus of its host galaxy; the spectrum shows a persistent blackbody temperature T ≳ 20 000 K with broad H I and He II emission; and it peaks at a blackbody luminosit…

2019 Monthly Notices of the Royal Astronomical Society
XMM-Newton 60