Search Publications

Resolving 3D Disk Orientation Using High-resolution Images: New Constraints on Circumgalactic Gas Inflows
DOI: 10.3847/1538-4357/ab58cd Bibcode: 2020ApJ...888...14H

Martin, Crystal L.; Ho, Stephanie H.

We constrain gas inflow speeds in star-forming galaxies with color gradients consistent with inside-out disk growth. Our method combines new measurements of disk orientation with previously described circumgalactic absorption in background quasar spectra. Two quantities, a position angle and an axis ratio, describe the projected shape of each gala…

2020 The Astrophysical Journal
eHST 25
Inferred time-scales for common envelope ejection using wide astrometric companions
DOI: 10.1093/mnras/staa833 Bibcode: 2020MNRAS.494.1448I

Igoshev, Andrei P.; Perets, Hagai B.; Michaely, Erez

Evolution of close binaries often proceeds through the common envelope stage. The physics of the envelope ejection (CEE) is not yet understood, and several mechanisms were suggested to be involved. These could give rise to different time-scales for the CEE mass-loss. In order to probe the CEE-time-scales we study wide companions to post-CE binarie…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 25
Labyrinth terrain on Titan
DOI: 10.1016/j.icarus.2020.113764 Bibcode: 2020Icar..34413764M

Malaska, Michael J.; Lopes, Rosaly M. C.; Solomonidou, Anezina +14 more

The Cassini/Huygens mission revealed a terrain type on Saturn's moon Titan of dissected, elevated plateaux with a high density of valleys named labyrinth terrain. We define four subtypes of labyrinth terrains: valleyed, polygonal, finely-dissected, and the possible outlier Kronin Labyrinth. We mapped the locations of all labyrinths imaged by Cassi…

2020 Icarus
Cassini 25
Discovery and characterization of the exoplanets WASP-148b and c. A transiting system with two interacting giant planets
DOI: 10.1051/0004-6361/202038296 Bibcode: 2020A&A...640A..32H

Bouchy, F.; Deleuil, M.; Queloz, D. +39 more

We present the discovery and characterization of WASP-148, a new extrasolar system that includes at least two giant planets. The host star is a slowly rotating inactive late-G dwarf with a V = 12 magnitude. The planet WASP-148b is a hot Jupiter of 0.72 RJup and 0.29 MJup that transits its host with an orbital period of 8.80 d…

2020 Astronomy and Astrophysics
Gaia 25
Heliospheric energetic neutral atoms: Non-stationary modelling and comparison with IBEX-Hi data
DOI: 10.1093/mnras/staa2862 Bibcode: 2020MNRAS.499..441B

Izmodenov, V. V.; Alexashov, D. B.; Baliukin, I. I.

The interstellar boundary explorer (IBEX) has been measuring fluxes of the energetic neutral atoms (ENAs) using the IBEX-Hi (0.3-6 keV) instrument since 2008. We have developed a numerical time-depended code to calculate globally distributed flux (GDF) of hydrogen ENAs employing both (1) 3D kinetic-MHD model of the global heliosphere and (2) recon…

2020 Monthly Notices of the Royal Astronomical Society
SOHO 25
Star catalog position and proper motion corrections in asteroid astrometry II: The Gaia era
DOI: 10.1016/j.icarus.2019.113596 Bibcode: 2020Icar..33913596E

Eggl, Siegfried; Chesley, Steven R.; Farnocchia, Davide +1 more

Astrometric positions of moving objects in the Solar System have been measured using a variety of star catalogs in the past. Previous work has shown that systematic errors in star catalogs can affect the accuracy of astrometric observations. That, in turn, can influence the resulting orbit fits for minor planets. In order to quantify these systema…

2020 Icarus
Gaia 25
Clustering with JWST: Constraining galaxy host halo masses, satellite quenching efficiencies, and merger rates at z = 4-10
DOI: 10.1093/mnras/staa324 Bibcode: 2020MNRAS.493.1178E

Stark, Daniel P.; Endsley, Ryan; Rieke, Marcia +5 more

Galaxy clustering measurements can be used to constrain many aspects of galaxy evolution, including galaxy host halo masses, satellite quenching efficiencies, and merger rates. We simulate JWST galaxy clustering measurements at z ∼ 4-10 by utilizing mock galaxy samples produced by an empirical model, the UNIVERSEMACHINE. We also adopt the survey f…

2020 Monthly Notices of the Royal Astronomical Society
eHST 25
Separation between RR Lyrae and type II Cepheids and their importance for a distance determination: the case of omega Cen
DOI: 10.1051/0004-6361/202039145 Bibcode: 2020A&A...644A..95B

Salaris, M.; Mateo, M.; Marinoni, S. +11 more

The separation between RR Lyrae (RRLs) and type II Cepheid (T2Cs) variables based on their period is debated. Both types of variable stars are distance indicators, and we aim to promote the use of T2Cs as distance indicators in synergy with RRLs. We adopted new and existing optical and near-infrared (NIR) photometry of ω Cen to investigate several…

2020 Astronomy and Astrophysics
Gaia 25
The Spectroscopic Follow-up of the QUBRICS Bright Quasar Survey
DOI: 10.3847/1538-4365/abafc1 Bibcode: 2020ApJS..250...26B

Grazian, Andrea; Boutsia, Konstantina; Amorin, Ricardo +11 more

We present the results of the spectroscopic follow-up of the QUasars as BRIght beacons for Cosmology in the Southern Hemisphere (QUBRICS; Calderone et al. 2019) survey. The selection method is based on a machine-learning approach applied to photometric catalogs, covering an area of ∼12,400 deg2 in the Southern Hemisphere. The spectrosco…

2020 The Astrophysical Journal Supplement Series
Gaia 25
Forward Modeling of Double Neutron Stars: Insights from Highly Offset Short Gamma-Ray Bursts
DOI: 10.3847/1538-4357/abc266 Bibcode: 2020ApJ...904..190Z

Fong, Wen-fai; Zevin, Michael; Kalogera, Vicky +3 more

We present a detailed analysis of two well-localized, highly offset short gamma-ray bursts—GRB 070809 and GRB 090515—investigating the kinematic evolution of their progenitors from compact object formation until merger. Calibrating to observations of their most probable host galaxies, we construct semi-analytic galactic models that account for sta…

2020 The Astrophysical Journal
eHST 25