Search Publications

Single metal-poor ultra compact dwarf galaxy at one kiloparsec distance from the low-mass elliptical galaxy FCC 47
DOI: 10.1051/0004-6361/201834941 Bibcode: 2019A&A...625A..50F

Fahrion, Katja; Alfaro-Cuello, Mayte; van de Ven, Glenn +7 more

Context. Photometric surveys of galaxy clusters have revealed a large number of ultra compact dwarfs (UCDs) around predominantly massive elliptical galaxies. Their origin is still debated as some UCDs are considered to be the remnant nuclei of stripped dwarf galaxies while others seem to mark the high-mass end of the star cluster population.

2019 Astronomy and Astrophysics
eHST 19
A Code for Robust Astrometric Solution of Astronomical Images
DOI: 10.1088/1538-3873/ab04df Bibcode: 2019PASP..131e4504O

Ofek, E. O.

I present a software tool for solving the astrometry of astronomical images. The code puts emphasis on robustness against failures for correctly matching the sources in the image to a reference catalog, and on the stability of the solutions over the field of view (e.g., using orthogonal polynomials for the fitted transformation). The code was test…

2019 Publications of the Astronomical Society of the Pacific
Gaia 18
Modelling of Mg II lines in solar prominences
DOI: 10.1051/0004-6361/201833132 Bibcode: 2019A&A...625A..30L

Labrosse, N.; Levens, P. J.

Context. Observations of the Mg II h and k lines in solar prominences with IRIS reveal a wide range of line shapes from simple non-reversed profiles to typical double-peaked reversed profiles, and with many other possible complex line shapes. The physical conditions responsible for this variety are not well understood.
Aims: Our aim is to und…

2019 Astronomy and Astrophysics
IRIS 18
Raised Rims Around Titan's Sharp-Edged Depressions
DOI: 10.1029/2018GL078099 Bibcode: 2019GeoRL..46.5846B

Lunine, J. I.; Hayes, A. G.; Lopes, R. M. C. +6 more

We perform a systematic survey of Titan's sharp-edged depressions (SEDs) using a combination of Cassini synthetic aperture radar images and delay-Doppler processed altimetry. We identify a characteristic bright-dark pattern around 172 SEDs that correlates with elevated features only resolved with the highest resolution topographic data. We find th…

2019 Geophysical Research Letters
Cassini 18
Formation of a New Great Dark Spot on Neptune in 2018
DOI: 10.1029/2019GL081961 Bibcode: 2019GeoRL..46.3108S

Simon, A. A.; Wong, M. H.; Hsu, A. I.

For the first time, Hubble Space Telescope visible-wavelength imaging shows the formation history of a dark vortex on Neptune. A new northern Great Dark Spot (NDS-2018) was discovered in September and November 2018 images, spanning roughly 12° of latitude and 27° in longitude (11,000 × 5,000 km) at 23°N planetographic latitude. NDS-2018 is similar…

2019 Geophysical Research Letters
eHST 18
Hot exozodiacal dust: an exocometary origin?
DOI: 10.1051/0004-6361/201935250 Bibcode: 2019A&A...626A...2S

Augereau, J. -C.; Sezestre, É.; Thébault, P.

Context. Near- and mid-infrared interferometric observations have revealed populations of hot and warm dust grains populating the inner regions of extrasolar planetary systems. These are known as exozodiacal dust clouds, or exozodis, reflecting the similarity with the solar system's zodiacal cloud. Radiative transfer models have constrained the du…

2019 Astronomy and Astrophysics
Gaia 18
Neutral carbon and highly excited CO in a massive star-forming main sequence galaxy at z = 2.2
DOI: 10.1051/0004-6361/201935148 Bibcode: 2019A&A...628A.104B

Daddi, Emanuele; Aravena, Manuel; Decarli, Roberto +5 more

We used the Plateau De Bure Interferometer to observe multiple CO and neutral carbon transitions in a z = 2.2 main sequence disk galaxy, BX610. Our observation of CO(7-6), CO(4-3), and both far-infrared (FIR) [CI] lines complements previous observations of Hα and low-J CO, and reveals a galaxy that is vigorously forming stars with UV fields (Log(G…

2019 Astronomy and Astrophysics
eHST 18
A Closer Look at Some Gas-phase Depletions in the ISM: Trends for O, Ge, and Kr versus {F}_{* }, f(H2), and Starlight Intensity
DOI: 10.3847/1538-4357/aafe81 Bibcode: 2019ApJ...872...55J

Jenkins, Edward B.

In a survey of archived ultraviolet spectra of 100 stars recorded by the echelle spectrograph of the Space Telescope Imaging Spectrograph on the Hubble Space Telescope, we measure the strengths of the weak absorption features of O I, Ge II, and Kr I in the interstellar medium. Our objective is to undertake an investigation that goes beyond earlier…

2019 The Astrophysical Journal
eHST 18
Compositional variations of Titan's impact craters indicates active surface erosion
DOI: 10.1016/j.icarus.2018.12.007 Bibcode: 2019Icar..321..508W

Janssen, M. A.; Cassini Radar Team; Werynski, A. +2 more

Titan, the only moon in the solar system with a considerable atmosphere, is host to a variety of exogenic processes that shape its surface. These processes form features that are quite similar to features on Earth, including sand dunes, rivers, and lakes. The combination of a thick atmosphere and active surface processes also leads to a scarcity o…

2019 Icarus
Cassini 18
The water line emission and ortho-to-para ratio in the Orion Bar photon-dominated region
DOI: 10.1051/0004-6361/201935402 Bibcode: 2019A&A...632A...8P

Le Petit, F.; Roueff, E.; Lis, D. C. +2 more

Context. The ortho-to-para ratio (OPR) of water in the interstellar medium (ISM) is often assumed to be related to the formation temperature of water molecules, making it a potentially interesting tracer of the thermal history of interstellar gas.
Aims: A very low OPR of 0.1-0.5 was previously reported in the Orion Bar photon-dominated region…

2019 Astronomy and Astrophysics
Herschel 18