Search Publications

X-ray spectra of the Fe-L complex
DOI: 10.1051/0004-6361/201833860 Bibcode: 2019A&A...627A..51G

Raassen, A. J. J.; Gu, Liyi; Mao, Junjie +7 more

The Hitomi results on the Perseus cluster have led to improvements in our knowledge of atomic physics that are crucial for the precise diagnostic of hot astrophysical plasma observed with high-resolution X-ray spectrometers. However, modeling uncertainties remains, both within but especially beyond Hitomi's spectral window. A major challenge in sp…

2019 Astronomy and Astrophysics
XMM-Newton 31
The scattered disc of HR 8799
DOI: 10.1093/mnras/sty3160 Bibcode: 2019MNRAS.483..332G

Booth, Mark; Krivov, Alexander V.; Löhne, Torsten +1 more

HR 8799 is a young F0-type star with four directly imaged giant planets and two debris belts, one located exterior and another one interior to the region occupied by the planetary orbits. Not only having an architecture similar to that of our Solar system but also revealing dissimilarities such as high masses of planets, a huge radial extent, and …

2019 Monthly Notices of the Royal Astronomical Society
AKARI Gaia Herschel 31
The Formation Conditions of the Wide Binary Class 0 Protostars within BHR 71
DOI: 10.3847/1538-4357/aaef87 Bibcode: 2019ApJ...870...81T

Bourke, Tyler L.; Codella, Claudio; Chen, Xuepeng +7 more

We present a characterization of the binary protostar system that is forming within a dense core in the isolated dark cloud BHR71. The pair of protostars, IRS1 and IRS2, are both in the Class 0 phase, determined from observations that resolve the sources from 1 µm out to 250 µm and from 1.3 mm to 1.3 cm. The resolved observations enabl…

2019 The Astrophysical Journal
Herschel 31
Testing dark matter with Cherenkov light — prospects of H.E.S.S. and CTA for exploring minimal supersymmetry
DOI: 10.1007/JHEP10(2019)043 Bibcode: 2019JHEP...10..043H

Moulin, Emmanuel; Hryczuk, Andrzej; Jodłowski, Krzysztof +4 more

We provide an updated and improved study of the prospects of the H.E.S.S. and Cherenkov Telescope Array (CTA) experiments in testing neutralino dark matter in the Minimal Supersymmetric Standard Model with nine free parameters (p9MSSM). We include all relevant experimental constraints and theoretical developments, in particular a calculation of th…

2019 Journal of High Energy Physics
Gaia 31
Gas velocity structure of the Orion A integral-shaped filament
DOI: 10.1093/mnras/stz2512 Bibcode: 2019MNRAS.489.4771G

Stutz, Amelia M.; González Lobos, Vale

We present analysis of the gas kinematics of the integral-shaped filament (ISF) in Orion A using four different molecular lines, 12CO (1-0), 13CO (1-0), NH3 (1,1), and N2H+ (1-0). We describe our method to visualize the position-velocity (PV) structure using the intensity-weighted line velocit…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 31
Tracing Hercules in Galactic azimuth with Gaia DR2
DOI: 10.1051/0004-6361/201936455 Bibcode: 2019A&A...632A.107M

Monari, G.; Siebert, A.; Famaey, B. +4 more

The second data release of the Gaia mission has revealed, in stellar velocity and action space, multiple ridges, the exact origin of which is still debated. Recently, we demonstrated that a large Galactic bar with pattern speed 39 km s-1 kpc-1 creates most of the observed ridges. Among these ridges, the Hercules moving group …

2019 Astronomy and Astrophysics
Gaia 31
Star-forming clumps in the Lyman Alpha Reference Sample of galaxies - I. Photometric analysis and clumpiness
DOI: 10.1093/mnras/stz1337 Bibcode: 2019MNRAS.487.4238M

Hayes, Matthew; Östlin, Göran; Melinder, Jens +4 more

We study young star-forming clumps on physical scales of 10-500 pc in the Lyman-Alpha Reference Sample (LARS), a collection of low-redshift (z = 0.03-0.2) UV-selected star-forming galaxies. In each of the 14 galaxies of the sample, we detect clumps for which we derive sizes and magnitudes in five UV-optical filters. The final sample includes ∼1400…

2019 Monthly Notices of the Royal Astronomical Society
eHST 31
Mean density inversions for red giants and red clump stars
DOI: 10.1093/mnras/sty2346 Bibcode: 2019MNRAS.482.2305B

Reese, D. R.; Eggenberger, P.; Bossini, D. +8 more

Since the CoRoT and Kepler missions, the availability of high-quality seismic spectra for red giants has made them the standard clocks and rulers for Galactic Archeology. With the expected excellent data from the TESS and PLATO missions, red giants will again play a key role in Galactic studies and stellar physics, thanks to the precise masses and…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 31
Organic molecules in the protoplanetary disk of DG Tauri revealed by ALMA
DOI: 10.1051/0004-6361/201834475 Bibcode: 2019A&A...623L...6P

Kamp, I.; Podio, L.; Bacciotti, F. +10 more

Context. Planets form in protoplanetary disks and inherit their chemical compositions.
Aims: It is thus crucial to map the distribution and investigate the formation of simple organics, such as formaldehyde and methanol, in protoplanetary disks.
Methods: We analyze ALMA observations of the nearby disk-jet system around the T Tauri star D…

2019 Astronomy and Astrophysics
Gaia 31
A Secondary Fan-spine Magnetic Structure in Active Region 11897
DOI: 10.3847/1538-4357/aaf4f4 Bibcode: 2019ApJ...871....4H

Hou, Yijun; Li, Ting; Yang, Shuhong +1 more

Fan-spine is a special topology in solar atmosphere and is closely related to magnetic null point, as well as circular-ribbon flares, which can provide important information for understanding the intrinsic 3D nature of solar flares. However, the fine structure within the fan has rarely been investigated. In present paper, we investigate a secondar…

2019 The Astrophysical Journal
IRIS 31