Search Publications

The Colors and Sizes of Recently Quenched Galaxies: A Result of Compact Starburst before Quenching
DOI: 10.3847/1538-4357/ab5fd9 Bibcode: 2020ApJ...888...77W

Bell, Eric F.; D'Eugenio, Francesco; Franx, Marijn +11 more

We analyze the colors and sizes of 32 quiescent (UVJ-selected) galaxies with strong Balmer absorption (EW(Hδ) ≥ 4 Å) at z ∼ 0.8 drawn from DR2 of the LEGA-C survey to test the hypothesis that these galaxies experienced compact, central starbursts before quenching. These recently quenched galaxies, usually referred to as post-starburst galaxies, sp…

2020 The Astrophysical Journal
eHST 46
A closer look at the spur, blob, wiggle, and gaps in GD-1
DOI: 10.1093/mnras/staa917 Bibcode: 2020MNRAS.494.5315D

Gieles, M.; Erkal, D.; de Boer, T. J. L.

The GD-1 stream is one of the longest and coldest stellar streams discovered to date, and one of the best objects for constraining the dark matter properties of the Milky Way. Using data from Gaia DR2, we study the proper motions (PMs), distance, morphology, and density of the stream to uncover small-scale perturbations. The PM cleaned data show a…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 46
Clouds of Fluffy Aggregates: How They Form in Exoplanetary Atmospheres and Influence Transmission Spectra
DOI: 10.3847/1538-4357/ab44bd Bibcode: 2020ApJ...891..131O

Okuzumi, Satoshi; Tazaki, Ryo; Ohno, Kazumasa

Transmission spectrum surveys have suggested the ubiquity of high-altitude clouds in exoplanetary atmospheres. Theoretical studies have investigated the formation processes of the high-altitude clouds; however, cloud particles have been commonly approximated as compact spheres, which is not always true for solid mineral particles that likely const…

2020 The Astrophysical Journal
eHST 46
The unusual broad-band X-ray spectral variability of NGC 1313 X-1 seen with XMM-Newton, Chandra, and NuSTAR
DOI: 10.1093/mnras/staa1129 Bibcode: 2020MNRAS.494.6012W

Harrison, F. A.; Stern, D.; Fabian, A. C. +19 more

We present results from the major coordinated X-ray observing programme on the ULX NGC 1313 X-1 performed in 2017, combining XMM-Newton, Chandra, and NuSTAR, focusing on the evolution of the broad-band (∼0.3-30.0 keV) continuum emission. Clear and unusual spectral variability is observed, but this is markedly suppressed above ∼10-15 keV, qualitati…

2020 Monthly Notices of the Royal Astronomical Society
XMM-Newton 46
Searching for ultra-fast outflows in AGN using variability spectra
DOI: 10.1093/mnras/staa265 Bibcode: 2020MNRAS.493.1088I

Schartel, N.; Santos-Lleó, M.; Buisson, D. J. K. +9 more

We present a qualitative search for ultra-fast outflows (UFOs) in excess variance spectra of radio-quiet active galactic nuclei (AGNs). We analyse 42 sources from the spectroscopic UFO detection sample, and an additional 22 different sources from the variability sample. A total of 58 sources have sufficient observational data from XMM-Newton EPIC-…

2020 Monthly Notices of the Royal Astronomical Society
XMM-Newton 46
Investigating the Effect of Galaxy Interactions on the Enhancement of Active Galactic Nuclei at 0.5 < z < 3.0
DOI: 10.3847/1538-4357/abbf59 Bibcode: 2020ApJ...904..107S

Hathi, Nimish P.; Kartaltepe, Jeyhan S.; Kocevski, Dale D. +30 more

Galaxy interactions and mergers are thought to play an important role in the evolution of galaxies. Studies in the nearby universe show a higher fraction of active galactic nuclei (AGNs) in interacting and merging galaxies than in their isolated counterparts, indicating that such interactions are important contributors to black hole growth. To inv…

2020 The Astrophysical Journal
eHST 46
Exploring the Evolution of Stellar Rotation Using Galactic Kinematics
DOI: 10.3847/1538-3881/ab91b2 Bibcode: 2020AJ....160...90A

Angus, Ruth; Foreman-Mackey, Daniel; van Saders, Jennifer +9 more

The rotational evolution of cool dwarfs is poorly constrained after ∼1-2 Gyr due to a lack of precise ages and rotation periods for old main-sequence stars. In this work, we use velocity dispersion as an age proxy to reveal the temperature-dependent rotational evolution of low-mass Kepler dwarfs and demonstrate that kinematic ages could be a usefu…

2020 The Astronomical Journal
Gaia 46
Revived fossil plasma sources in galaxy clusters
DOI: 10.1051/0004-6361/201936560 Bibcode: 2020A&A...634A...4M

Di Gennaro, G.; Brunetti, G.; Shimwell, T. W. +10 more

It is well established that particle acceleration by shocks and turbulence in the intra-cluster medium can produce cluster-scale synchrotron emitting sources. However, the detailed physics of these particle acceleration processes is still not well understood. One of the main open questions is the role of fossil relativistic electrons that have bee…

2020 Astronomy and Astrophysics
XMM-Newton 46
ALMA Observations of Multiple CO and C Lines toward the Active Galactic Nucleus of NGC 7469: An X-Ray-dominated Region Caught in the Act
DOI: 10.3847/1538-4357/ab9cb1 Bibcode: 2020ApJ...898...75I

Baba, Shunsuke; Meier, David S.; Turner, Jean L. +15 more

We used the Atacama Large Millimeter/submillimeter Array to map 12CO(J = 1-0), 12CO(J = 2-1), 12CO(J = 3-2), 13CO(J = 2-1), and [C I](3P1-3P0) emission lines around the type 1 active galactic nucleus (AGN) of NGC 7469 (z = 0.0164) at ∼100 pc resolutions. The CO…

2020 The Astrophysical Journal
eHST 46
The soft X-ray excess: NLS1s versus BLS1s
DOI: 10.1093/mnras/stz3005 Bibcode: 2020MNRAS.491..532G

Gliozzi, Mario; Williams, James K.

The soft X-ray excess - the excess of X-rays below 2 keV with respect to the extrapolation of the hard X-ray spectral continuum model - is a very common feature among type 1 active galactic nuclei (AGNs); yet the nature of the soft X-ray excess is still poorly understood and hotly debated. To shed some light on this issue, we have measured in a mo…

2020 Monthly Notices of the Royal Astronomical Society
XMM-Newton 46