Search Publications

Modeling ionized gas in low-metallicity environments: the Local Group dwarf galaxy IC 10
DOI: 10.1051/0004-6361/201833776 Bibcode: 2019A&A...622A.119P

Lebouteiller, V.; Madden, S. C.; Galliano, F. +9 more

Context. Star formation activity is an important driver of galaxy evolution and is influenced by the physical properties of the interstellar medium. Dwarf galaxies allow us to understand how the propagation of radiation and the physical conditions of the different ISM phases are affected by the low-metallicity environment.
Aims: Our objective…

2019 Astronomy and Astrophysics
Herschel 22
Terrestrial ion escape and relevant circulation in space
DOI: 10.5194/angeo-37-1197-2019 Bibcode: 2019AnGeo..37.1197Y

Yamauchi, Masatoshi

Observations of the terrestrial ion escape to space and the transport of escaping ions in the magnetosphere are reviewed, with the main stress on subjects that were not covered in reviews over past 2 decades, during which Cluster has significantly improved our knowledge of them. Here, outflowing ions from the ionosphere are classified in terms of …

2019 Annales Geophysicae
Cluster 22
Collimated radiation in SS 433. Constraints from spatially resolved optical jets and Cloudy modeling of the optical bullets
DOI: 10.1051/0004-6361/201834747 Bibcode: 2019A&A...624A.127W

Dexter, Jason; Waisberg, Idel; Dubus, Guillaume +2 more

Context. The microquasar SS 433 is well known for its precessing, relativistic, and highly collimated baryonic jets, which manifest in its optical spectrum as pairs of hydrogen and helium emission lines moving with large Doppler shifts. Depending on their heating mechanism, the optical jet bullets may serve as a probe of the collimated radiation c…

2019 Astronomy and Astrophysics
Gaia 22
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
Spin Parity of Spiral Galaxies. I. Corroborative Evidence for Trailing Spirals
DOI: 10.3847/1538-4357/ab4a18 Bibcode: 2019ApJ...886..133I

Tadaki, Ken-ichi; Iye, Masanori; Fukumoto, Hideya

Whether the spiral structure of galaxies is trailing or leading has been a subject of debate. We present a new spin parity catalog of 146 spiral galaxies that lists the following three pieces of information: whether the spiral structure observed on the sky is S-wise or Z-wise; which side of the minor axis of the galaxy is darker and redder, based …

2019 The Astrophysical Journal
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
Evidence for mass accretion driven by spiral shocks onto the white dwarf in SDSS J123813.73-033933.0
DOI: 10.1093/mnras/sty3174 Bibcode: 2019MNRAS.483.1080P

Reichart, D. E.; Wang, L.; Knigge, C. +21 more

We present high-time-resolution photometry and phase-resolved spectroscopy of the short-period ({P_orb}= 80.52 min) cataclysmic variable SDSS J123813.73-033933.0, observed with the Hubble Space Telescope (HST), the Kepler/K2 mission, and the Very Large Telescope (VLT). We also report observations of the first detected superoutburst. SDSS J1238-033…

2019 Monthly Notices of the Royal Astronomical Society
Gaia eHST 22
Variable dust emission by WC type Wolf-Rayet stars observed in the NEOWISE-R survey
DOI: 10.1093/mnras/stz1784 Bibcode: 2019MNRAS.488.1282W

Williams, P. M.

Photometry at 3.4 and 4.6 {µ m} of 128 Population I WC type Wolf-Rayet stars in the Galaxy and 12 in the Large Magellanic Cloud (LMC) observed in the WISE NEOWISE-R survey was searched for evidence of circumstellar dust emission and its variation. Infrared spectral energy distributions (SEDs) were assembled, making use of archival r, i, Z, a…

2019 Monthly Notices of the Royal Astronomical Society
AKARI Gaia 22
Manifestations of Three-dimensional Magnetic Reconnection in an Eruption of a Quiescent Filament: Filament Strands Turning to Flare Loops
DOI: 10.3847/1538-4357/ab4519 Bibcode: 2019ApJ...885...83L

Aulanier, Guillaume; Dudík, Jaroslav; Lörinčík, Juraj

We report on observations of the conversion of bright filament strands into flare loops during the 2012 August 31 filament eruption. Prior to the eruption, individual bright strands composing one of the legs of the filament were observed in the 171 Å filter channel data of the Atmospheric Imaging Assembly. After the onset of the eruption, one of t…

2019 The Astrophysical Journal
Hinode 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