Search Publications

Are the spiral arms in the MWC 758 protoplanetary disc driven by a companion inside the cavity?
DOI: 10.1093/mnras/staa2468 Bibcode: 2020MNRAS.498..639C

Pinte, Christophe; Christiaens, Valentin; van der Marel, Nienke +4 more

Spiral arms in protoplanetary discs are thought to be linked to the presence of companions. We test the hypothesis that the double spiral arm morphology observed in the transition disc MWC 758 can be generated by an ≈10MJup companion on an eccentric orbit internal to the spiral arms. Previous studies on MWC 758 have assumed an external …

2020 Monthly Notices of the Royal Astronomical Society
Gaia 38
Chemodynamics of green pea galaxies - I. Outflows and turbulence driving the escape of ionizing photons and chemical enrichment
DOI: 10.1093/mnras/staa851 Bibcode: 2020MNRAS.494.3541H

Amorín, R.; Pérez-Montero, E.; Vílchez, J. M. +6 more

We investigate the ionized gas kinematics, physical properties, and chemical abundances of Sloan Digital Sky Survey J142947, a Green Pea galaxy at redshift z∼ 0.17 with strong, double-peak Ly α emission and indirect evidence of Lyman continuum (LyC) leakage. Using high-dispersion spectroscopy, we perform a multicomponent analysis of emission-line …

2020 Monthly Notices of the Royal Astronomical Society
eHST 38
The surface distributions of the production of the major volatile species, H2O, CO2, CO and O2, from the nucleus of comet 67P/Churyumov-Gerasimenko throughout the Rosetta Mission as measured by the ROSINA double focusing mass spectrometer
DOI: 10.1016/j.icarus.2019.113421 Bibcode: 2020Icar..33513421C

Hansen, Kenneth C.; Altwegg, Kathrin; Rubin, Martin +12 more

The Rosetta Orbiter Spectrometer for Ion and Neutral Analysis (ROSINA) suite of instruments operated throughout the over two years of the Rosetta mission operations in the vicinity of comet 67P/Churyumov-Gerasimenko. It measured gas densities and composition throughout the comet's atmosphere, or coma. Here we present two-years' worth of measuremen…

2020 Icarus
Rosetta 38
Constraining the Kilonova Rate with Zwicky Transient Facility Searches Independent of Gravitational Wave and Short Gamma-Ray Burst Triggers
DOI: 10.3847/1538-4357/abbf4c Bibcode: 2020ApJ...904..155A

Kulkarni, S. R.; Cenko, S. Bradley; Duev, Dmitry A. +34 more

The first binary neutron star merger, GW170817, was accompanied by a radioactivity-powered optical/infrared transient called a kilonova. To date, no compelling kilonova has been found in all-sky optical surveys, independently of short gamma-ray burst and gravitational-wave triggers. In this work, we searched the first 23 months of the Zwicky Trans…

2020 The Astrophysical Journal
Gaia 38
LEGUS and Hα-LEGUS Observations of Star Clusters in NGC 4449: Improved Ages and the Fraction of Light in Clusters as a Function of Age
DOI: 10.3847/1538-4357/ab59e5 Bibcode: 2020ApJ...889..154W

Grebel, Eva K.; Smith, Linda J.; Aloisi, Alessandra +17 more

We present a new catalog and results for the cluster system of the starburst galaxy NGC 4449, based on multiband imaging observations taken as part of the LEGUS and Hα-LEGUS surveys. We improve the spectral energy fitting method used to estimate cluster ages, and find that the results, particularly for older clusters, are in better agre…

2020 The Astrophysical Journal
eHST 38
Probing the Nature of High-redshift Weak Emission Line Quasars: A Young Quasar with a Starburst Host Galaxy
DOI: 10.3847/1538-4357/abb9a6 Bibcode: 2020ApJ...903...34A

Neeleman, Marcel; Walter, Fabian; Simcoe, Robert A. +15 more

We present the discovery of PSO J083.8371+11.8482, a weak emission line quasar with extreme star formation rate at z = 6.3401. This quasar was selected from Pan-STARRS1, UHS, and unWISE photometric data. Gemini/GNIRS spectroscopy follow-up indicates a Mg II-based black hole mass of ${M}_{\mathrm{BH}}=\left({2.0}_{-0.4}^{+0.7}\right)\times {10}^{9}…

2020 The Astrophysical Journal
eHST 38
Retrieval of the d/sdL7+T7.5p Binary SDSS J1416+1348AB
DOI: 10.3847/1538-4357/abbee2 Bibcode: 2020ApJ...905...46G

Gonzales, Eileen C.; Marley, Mark S.; Faherty, Jacqueline K. +5 more

We present the distance-calibrated spectral energy distribution (SED) of the d/sdL7 SDSS J14162408+1348263A (J1416A) and an updated SED for SDSS J14162408+1348263B (J1416B). We also present the first retrieval analysis of J1416A using the Brewster retrieval code base and the second retrieval of J1416B. We find that the primary is best fit by a non…

2020 The Astrophysical Journal
Gaia 38
Internal motions in OB associations with Gaia DR2
DOI: 10.1093/mnras/staa454 Bibcode: 2020MNRAS.493.2339M

Melnik, A. M.; Dambis, A. K.

We study the motions inside 28 OB associations with the use of Gaia DR2 proper motions. The average velocity dispersion calculated for 28 OB associations including more than 20 stars with Gaia DR2 proper motion is σV = 4.5 km s-1. The median virial and stellar masses of OB associations are Mvir = 8.9 × 105

2020 Monthly Notices of the Royal Astronomical Society
Gaia 38
The CO-dark molecular gas mass in 30 Doradus
DOI: 10.1093/mnras/staa1106 Bibcode: 2020MNRAS.494.5279C

Lebouteiller, Vianney; Lee, Min-Young; Kruijssen, J. M. Diederik +16 more

Determining the efficiency with which gas is converted into stars in galaxies requires an accurate determination of the total reservoir of molecular gas mass. However, despite being the most abundant molecule in the Universe, H2 is challenging to detect through direct observations and indirect methods have to be used to estimate the tot…

2020 Monthly Notices of the Royal Astronomical Society
Herschel 38
MIRACLES: atmospheric characterization of directly imaged planets and substellar companions at 4-5 µm. II. Constraints on the mass and radius of the enshrouded planet PDS 70 b
DOI: 10.1051/0004-6361/202038878 Bibcode: 2020A&A...644A..13S

Quanz, S. P.; Todorov, K. O.; Stolker, T. +4 more

The circumstellar disk of PDS 70 hosts two forming planets, which are actively accreting gas from their environment. The physical and chemical characteristics of these planets remain ambiguous due to their unusual spectral appearance compared to more evolved objects. In this work, we report the first detection of PDS 70 b in the Brα and M' filters…

2020 Astronomy and Astrophysics
Gaia 38