Search Publications

The Holy Grail: A road map for unlocking the climate record stored within Mars' polar layered deposits
DOI: 10.1016/j.pss.2020.104841 Bibcode: 2020P&SS..18404841S

Horgan, Briony; Byrne, Shane; Zacny, Kris +35 more

In its polar layered deposits (PLD), Mars possesses a record of its recent climate, analogous to terrestrial ice sheets containing climate records on Earth. Each PLD is greater than 2 km thick and contains thousands of layers, each containing information on the climatic and atmospheric state during its deposition, creating a climate archive. With …

2020 Planetary and Space Science
MEx 28
Molecular gas inflows and outflows in ultraluminous infrared galaxies at z ∼ 0.2 and one QSO at z = 6.1
DOI: 10.1051/0004-6361/201937109 Bibcode: 2020A&A...633L...4H

Lutz, D.; Genzel, R.; Maiolino, R. +12 more


Aims: Our aim is to search for and characterize inflows and outflows of molecular gas in four ultraluminous infrared galaxies (ULIRGs; LIR > 1012L) at z ∼ 0.2-0.3 and one distant quasi-stellar object (QSO) at z = 6.13.
Methods: We used Herschel/PACS and ALMA Band 7 observations of the hydroxyl molecul…

2020 Astronomy and Astrophysics
Herschel 28
The Structure of Tidal Disruption Event Host Galaxies on Scales of Tens to Thousands of Parsecs
DOI: 10.3847/1538-4357/ab7450 Bibcode: 2020ApJ...891...93F

Zabludoff, Ann I.; French, K. Decker; van Velzen, Sjoert +5 more

We explore the galaxy structure of four tidal disruption event (TDE) host galaxies on 30 pc to kiloparsec scales using Hubble Space Telescope WFC3 multiband imaging. The star formation histories of these hosts are diverse, including one post-starburst galaxy (ASASSN-14li), two hosts with recent weak starbursts (ASASSN-14ae and iPTF15af), and one e…

2020 The Astrophysical Journal
eHST 27
Strong Soft X-Ray Excess in 2015 XMM-Newton Observations of BL Lac OJ 287
DOI: 10.3847/1538-4357/ab65ee Bibcode: 2020ApJ...890...47P

Dewangan, G. C.; Pal, Main; Kushwaha, Pankaj +1 more

We report a strong soft X-ray excess in the BL Lacartae γ-ray blazar OJ 287 during long exposure in 2015 May, among two of the latest XMM-Newton observations performed in 2015 and 2018 May. In the case of the 2015 May observation, a log parabola model fits the EPIC-pn data well, while a log parabola plus a power law describes the overall simultane…

2020 The Astrophysical Journal
XMM-Newton 27
A Featureless Infrared Transmission Spectrum for the Super-puff Planet Kepler-79d
DOI: 10.3847/1538-3881/abb23a Bibcode: 2020AJ....160..201C

Deming, Drake; Madhusudhan, Nikku; Wakeford, Hannah R. +12 more

Extremely low-density planets ("super-puffs") are a small but intriguing subset of the transiting planet population. With masses in the super-Earth range (1 - 10 ${M}_{\oplus }$ ) and radii akin to those of giant planets (> 4 ${R}_{\oplus }$ ), their large envelopes may have been accreted beyond the water snow line and many appear to be suscept…

2020 The Astronomical Journal
eHST 27
Investigating the spectral age problem with powerful radio galaxies
DOI: 10.1093/mnras/stz3396 Bibcode: 2020MNRAS.491.5015M

Croston, Judith H.; Hardcastle, Martin J.; Mahatma, Vijay H. +3 more

The 'spectral age problem' is our systematic inability to reconcile the maximum cooling time of radiating electrons in the lobes of a radio galaxy with its age as modelled by the dynamical evolution of the lobes. While there are known uncertainties in the models that produce both age estimates, 'spectral' ages are commonly underestimated relative …

2020 Monthly Notices of the Royal Astronomical Society
XMM-Newton 27
Multiphase outflows in post-starburst E+A galaxies - II. A direct connection between the neutral and ionized outflow phases
DOI: 10.1093/mnras/staa1018 Bibcode: 2020MNRAS.494.5396B

Netzer, Hagai; Xavier Prochaska, J.; Baron, Dalya +1 more

Post-starburst E+A galaxies are systems that hosted a powerful starburst that was quenched abruptly. Simulations suggest that these systems provide the missing link between major merger ULIRGs and red and dead ellipticals, where AGN feedback is responsible for the expulsion or destruction of the molecular gas. However, many details remain unresolv…

2020 Monthly Notices of the Royal Astronomical Society
XMM-Newton 27
NuSTAR Perspective on High-redshift MeV Blazars
DOI: 10.3847/1538-4357/ab65f5 Bibcode: 2020ApJ...889..164M

Ajello, M.; Gasparrini, D.; Marchesi, S. +7 more

With bolometric luminosities exceeding 1048 erg s-1, powerful jets, and supermassive black holes at their center, MeV blazars are some of the most extreme sources in the universe. Recently, the Fermi-Large Area Telescope detected five new γ-ray emitting MeV blazars beyond redshift z = 3.1. With the goal of precisely character…

2020 The Astrophysical Journal
XMM-Newton 27
Spectroscopic characterization of the known O-star population in Cygnus OB2. Evidence of multiple star-forming bursts
DOI: 10.1051/0004-6361/202039015 Bibcode: 2020A&A...642A.168B

Lennon, D. J.; Herrero, A.; Comerón, F. +6 more

Context. Cygnus OB2 provides a unique insight into the high-mass stellar content in one of the largest groups of young massive stars in our Galaxy. Although several studies of its massive population have been carried out over the last decades, an extensive spectroscopic study of the whole known O-star population in the association is still lacking…

2020 Astronomy and Astrophysics
Gaia 27
Binary-induced spiral arms inside the disc cavity of AB Aurigae
DOI: 10.1093/mnras/staa1655 Bibcode: 2020MNRAS.496.2362P

Pinte, Christophe; Ribas, Álvaro; Macías, Enrique +5 more

In this work we demonstrate that the inner spiral structure observed in AB Aurigae can be created by a binary star orbiting inside the dust cavity. We find that a companion with a mass-ratio of 0.25, semimajor axis of 40 au, eccentricity of 0.5, and inclination of 90° produces gaseous spirals closely matching the ones observed in 12CO (…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 27