Search Publications

Young stellar populations in early-type dwarf galaxies. Occurrence, radial extent, and scaling relations
DOI: 10.1051/0004-6361/201935076 Bibcode: 2019A&A...625A..94H

Peletier, R. F.; Valentijn, E. A.; Hamraz, E. +3 more


Aims: To understand the stellar population content of early-type dwarf galaxies (dEs) and their environmental dependence, we compare the slopes and intrinsic scatter of color-magnitude relations (CMRs) for three nearby clusters, Fornax, Virgo, and Coma. Additionally, we present and compare internal color profiles of these galaxies to identify…

2019 Astronomy and Astrophysics
eHST 22
Massive dust clumps in the envelope of the red supergiant VY Canis Majoris
DOI: 10.1051/0004-6361/201935408 Bibcode: 2019A&A...627A.114K

Kamiński, T.

The envelope of the red supergiant VY CMa has long been considered an extreme example of episodic mass loss that is possibly taking place in other cool and massive evolved stars. Recent (sub-)millimeter observations of the envelope revealed the presence of massive dusty clumps within 800 mas of the star and reinforce the picture of drastic mass-lo…

2019 Astronomy and Astrophysics
eHST 22
Nature of a shell of young stars in the outskirts of the Small Magellanic Cloud
DOI: 10.1051/0004-6361/201936021 Bibcode: 2019A&A...631A..98M

Bell, Eric F.; Carballo-Bello, Julio A.; Grebel, Eva K. +36 more

Context. Understanding the evolutionary history of the Magellanic Clouds requires an in-depth exploration and characterization of the stellar content in their outer regions, which ultimately are key to tracing the epochs and nature of past interactions.
Aims: We present new deep images of a shell-like overdensity of stars in the outskirts of …

2019 Astronomy and Astrophysics
Gaia 22
Exploring the dimming event of RW Aurigae A through multi-epoch VLT/X-shooter spectroscopy
DOI: 10.1051/0004-6361/201834713 Bibcode: 2019A&A...625A..49K

Ray, T. P.; Coffey, D.; Natta, A. +6 more

Context. RW Aur A is a classical T Tauri star that has suddenly undergone three major dimming events since 2010. The reason for these dimming events is still not clear.
Aims: We aim to understand the dimming properties, examine accretion variability, and derive the physical properties of the inner disc traced by the CO ro-vibrational emission…

2019 Astronomy and Astrophysics
Gaia 22
Overview of non-transient γ-ray binaries and prospects for the Cherenkov Telescope Array
DOI: 10.1051/0004-6361/201936501 Bibcode: 2019A&A...631A.177C

Walter, R.; Sidoli, L.; La Palombara, N. +20 more


Aims: Despite recent progress in the field, there are still many open questions regarding γ-ray binaries. In this paper we provide an overview of non-transient γ-ray binaries and discuss how observations with the Cherenkov Telescope Array (CTA) will contribute to their study.
Methods: We simulated the spectral behaviour of the non-transi…

2019 Astronomy and Astrophysics
Gaia INTEGRAL 22
Stellar population astrophysics (SPA) with the TNG. GIANO-B spectroscopy of red supergiants in Alicante 7 and Alicante 10
DOI: 10.1051/0004-6361/201936283 Bibcode: 2019A&A...629A.117O

Dalessandro, E.; Rainer, M.; Bragaglia, A. +6 more


Aims: The Scutum complex in the inner disk of the Galaxy hosts a number of young clusters and associations of red supergiant stars that are heavily obscured by dust extinction. These stars are important tracers of the recent star formation and chemical enrichment history in the inner Galaxy.
Methods: Within the SPA Large Programme at the…

2019 Astronomy and Astrophysics
Gaia 22
Count-based imaging model for the Spectrometer/Telescope for Imaging X-rays (STIX) in Solar Orbiter
DOI: 10.1051/0004-6361/201935323 Bibcode: 2019A&A...624A.130M

Massa, Paolo; Piana, Michele; Benvenuto, Federico +1 more

The Spectrometer/Telescope for Imaging X-rays (STIX) will study solar flares across the hard X-ray window provided by the Solar Orbiter cluster. Similarly to the Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI), STIX is a visibility-based imaging instrument that will require Fourier-based image reconstruction methods. However, in this…

2019 Astronomy and Astrophysics
SolarOrbiter 22
Dust emissivity and absorption cross section in DustPedia late-type galaxies
DOI: 10.1051/0004-6361/201936314 Bibcode: 2019A&A...631A.102B

Bianchi, S.; Madden, S. C.; Galliano, F. +16 more


Aims: We compare the far-infrared to sub-millimetre dust emission properties measured in high Galactic latitude cirrus with those determined in a sample of 204 late-type DustPedia galaxies. The aim is to verify if it is appropriate to use Milky Way dust properties to derive dust masses in external galaxies.
Methods: We used Herschel obse…

2019 Astronomy and Astrophysics
Herschel 22
IFU investigation of possible Lyman continuum escape from Mrk 71/NGC 2366
DOI: 10.1051/0004-6361/201834838 Bibcode: 2019A&A...623A.145M

Östlin, Göran; Roth, Martin M.; Micheva, Genoveva +2 more

Context. Mrk 71/NGC 2366 is the closest green pea (GP) analog and candidate Lyman Continuum (LyC) emitter. Recently, 11 LyC-leaking GPs have been detected through direct observations of the ionizing continuum, making this the most abundant class of confirmed LyC-emitters at any redshift. High resolution, multiwavelength studies of GPs can lead to …

2019 Astronomy and Astrophysics
eHST 21
CHANG-ES. XIV. Cosmic-ray propagation and magnetic field strengths in the radio halo of NGC 4631
DOI: 10.1051/0004-6361/201834571 Bibcode: 2019A&A...632A..10M

Beck, Rainer; Kamieneski, Patrick; Irwin, Judith +13 more


Aims: NGC 4631 is an interacting galaxy that exhibits one of the largest, gaseous halos observed among edge-on galaxies. We aim to examine the synchrotron and cosmic-ray propagation properties of its disk and halo emission with new radio continuum data.
Methods: Radio continuum observations of NGC 4631 were performed with the Karl G. Jan…

2019 Astronomy and Astrophysics
Herschel 21