Search Publications

Testing the cosmic curvature at high redshifts: the combination of LSST strong lensing systems and quasars as new standard candles
DOI: 10.1093/mnras/staa1539 Bibcode: 2020MNRAS.496..708L

Zhang, Jia; Liu, Yuting; Cao, Shuo +3 more

The cosmic curvature, a fundamental parameter for cosmology could hold deep clues to inflation and cosmic origins. We propose an improved model-independent method to constrain the cosmic curvature by combining the constructed Hubble diagram of high-redshift quasars with galactic-scale strong lensing systems expected to be seen by the forthcoming L…

2020 Monthly Notices of the Royal Astronomical Society
eHST 43
Studying the Composition and Mineralogy of the Hermean Surface with the Mercury Radiometer and Thermal Infrared Spectrometer (MERTIS) for the BepiColombo Mission: An Update
DOI: 10.1007/s11214-020-00732-4 Bibcode: 2020SSRv..216..110H

Hiesinger, H.; Maturilli, A.; Helbert, J. +10 more

Launched onboard the BepiColombo Mercury Planetary Orbiter (MPO) in October 2018, the Mercury Radiometer and Thermal Infrared Spectrometer (MERTIS) is on its way to planet Mercury. MERTIS consists of a push-broom IR-spectrometer (TIS) and a radiometer (TIR), which operate in the wavelength regions of 7-14 µm and 7-40 µm, respectively. …

2020 Space Science Reviews
BepiColombo 43
DEATHSTAR: Nearby AGB stars with the Atacama Compact Array. I. CO envelope sizes and asymmetries: A new hope for accurate mass-loss-rate estimates
DOI: 10.1051/0004-6361/201936874 Bibcode: 2020A&A...640A.133R

Lindqvist, M.; Olofsson, H.; Sahai, R. +16 more

Context. This is the first publication from the DEATHSTAR project. The overall goal of the project is to reduce the uncertainties of the observational estimates of mass-loss rates from evolved stars on the Asymptotic Giant Branch (AGB). Aim. The aim in this first publication is to constrain the sizes of the 12CO emitting region from the…

2020 Astronomy and Astrophysics
Gaia 43
Ongoing flyby in the young multiple system UX Tauri
DOI: 10.1051/0004-6361/202038356 Bibcode: 2020A&A...639L...1M

Pinte, C.; Ménard, F.; van der Plas, G. +28 more

We present observations of the young multiple system UX Tauri to look for circumstellar disks and for signs of dynamical interactions. We obtained SPHERE/IRDIS deep differential polarization images in the J and H bands. We also used ALMA archival CO data. Large extended spirals are well detected in scattered light coming out of the disk of UX Tau …

2020 Astronomy and Astrophysics
Gaia 43
Modeling protoplanetary disk SEDs with artificial neural networks. Revisiting the viscous disk model and updated disk masses
DOI: 10.1051/0004-6361/202038352 Bibcode: 2020A&A...642A.171R

Sarro, L. M.; Ribas, Á.; Macías, E. +1 more

We model the spectral energy distributions (SEDs) of 23 protoplanetary disks in the Taurus-Auriga star-forming region using detailed disk models and a Bayesian approach. This is made possible by combining these models with artificial neural networks to drastically speed up their performance. Such a setup allows us to confront α-disk models with ob…

2020 Astronomy and Astrophysics
Gaia 43
Observation of the Second LIGO/Virgo Event Connected with a Binary Neutron Star Merger S190425z in the Gamma-Ray Range
DOI: 10.1134/S1063773719110057 Bibcode: 2020AstL...45..710P

Minaev, P. Yu.; Pozanenko, A. S.; Grebenev, S. A. +1 more

The results of observations of the gravitational-wave (GW) event S190425z recorded by the LIGO/Virgo detectors with the anti-coincidence shield (ACS) of the SPI gamma-ray spectrometer onboard the INTEGRAL observatory are presented. With a high probability (>99%) it was associated with a neutron star (NS) merger in a close binary system. This is…

2020 Astronomy Letters
INTEGRAL 43
Demographics of disks around young very low-mass stars and brown dwarfs in Lupus
DOI: 10.1051/0004-6361/201936913 Bibcode: 2020A&A...633A.114S

de Gregorio-Monsalvo, I.; Henning, T.; Pascucci, I. +15 more

We present new 890 µm continuum ALMA observations of five brown dwarfs (BDs) with infrared excess in Lupus I and III, which in combination with four previously observed BDs allowed us to study the millimeter properties of the full known BD disk population of one star-forming region. Emission is detected in five out of the nine BD disks. Dust…

2020 Astronomy and Astrophysics
Gaia 43
Size and Shape Constraints of (486958) Arrokoth from Stellar Occultations
DOI: 10.3847/1538-3881/ab6ced Bibcode: 2020AJ....159..130B

Dunham, David W.; Tanga, Paolo; Singer, Kelsi N. +130 more

We present the results from four stellar occultations by (486958) Arrokoth, the flyby target of the New Horizons extended mission. Three of the four efforts led to positive detections of the body, and all constrained the presence of rings and other debris, finding none. Twenty-five mobile stations were deployed for 2017 June 3 and augmented by fix…

2020 The Astronomical Journal
Gaia eHST 42
Precise mass and radius of a transiting super-Earth planet orbiting the M dwarf TOI-1235: a planet in the radius gap?
DOI: 10.1051/0004-6361/202038160 Bibcode: 2020A&A...639A.132B

Fridlund, M.; Rauer, H.; Amado, P. J. +81 more

We report the confirmation of a transiting planet around the bright weakly active M0.5 V star TOI-1235 (TYC 4384-1735-1, V ≈ 11.5 mag), whose transit signal was detected in the photometric time series of sectors 14, 20, and 21 of the TESS space mission. We confirm the planetary nature of the transit signal, which has a period of 3.44 d, by using p…

2020 Astronomy and Astrophysics
Gaia 42
Magnetic Field Dependence of Bipolar Magnetic Region Tilts on the Sun: Indication of Tilt Quenching
DOI: 10.3847/2041-8213/ab665c Bibcode: 2020ApJ...889L..19J

Banerjee, Dipankar; Jha, Bibhuti Kumar; Karak, Bidya Binay +1 more

The tilt of the bipolar magnetic region (BMR) is crucial in the Babcock-Leighton process for the generation of the poloidal magnetic field in the Sun. Based on the thin flux-tube model of the BMR formation, the tilt is believed to be caused by the Coriolis force acting on the rising flux tube of the strong toroidal magnetic field from the base of …

2020 The Astrophysical Journal
SOHO 42