Search Publications

L-GALAXIES 2020: The evolution of radial metallicity profiles and global metallicities in disc galaxies
DOI: 10.1093/mnras/stab741 Bibcode: 2021MNRAS.503.4474Y

White, Simon D. M.; Yates, Robert M.; Henriques, Bruno M. B. +5 more

We present a modified version of the L-GALAXIES2020 semi-analytic model of galaxy evolution, which includes significantly increased direct metal enrichment of the circumgalactic medium (CGM) by supernovae (SNe). These more metal-rich outflows do not require increased mass-loading factors, in contrast to some other galaxy evolution models. This mod…

2021 Monthly Notices of the Royal Astronomical Society
eHST 53
ALMA Measures Rapidly Depleted Molecular Gas Reservoirs in Massive Quiescent Galaxies at z ∼ 1.5
DOI: 10.3847/1538-4357/abcbf6 Bibcode: 2021ApJ...908...54W

Bezanson, Rachel; Brammer, Gabriel; Weiner, Benjamin +6 more

We present Atacama Large Millimeter/submillimeter Array (ALMA) CO(2-1) spectroscopy of six massive (log10 ${M}_{* }$ / ${M}_{\odot }$ > 11.3) quiescent galaxies at z ∼ 1.5. These data represent the largest sample using CO emission to trace molecular gas in quiescent galaxies above z > 1, achieving an average 3σ sensitivity of ${M}…

2021 The Astrophysical Journal
Gaia eHST 53
Turbulence in space plasmas: Who needs it?
DOI: 10.1063/5.0041540 Bibcode: 2021PhPl...28c2306M

Matthaeus, W. H.

The complex nonlinear dynamical phenomenon described as turbulence, is known to have a great impact on fluids, magnetohydrodynamic systems, and on plasmas. This paper reviews selected topics on turbulence in these systems, emphasizing the multiscale space-time properties of the turbulence cascade as it transfers energy from large scale reservoirs,…

2021 Physics of Plasmas
Cluster 53
pyUPMASK: an improved unsupervised clustering algorithm
DOI: 10.1051/0004-6361/202040252 Bibcode: 2021A&A...650A.109P

Moitinho, A.; Perren, G. I.; Pera, M. S. +2 more


Aims: We present pyUPMASK, an unsupervised clustering method for stellar clusters that builds upon the original UPMASK package. The general approach of this method makes it plausible to be applied to analyses that deal with binary classes of any kind as long as the fundamental hypotheses are met. The code is written entirely in Python and is …

2021 Astronomy and Astrophysics
Gaia 52
Photometric Dissection of Intracluster Light and Its Correlations with Host Cluster Properties
DOI: 10.3847/1538-4365/abcda6 Bibcode: 2021ApJS..252...27K

Schmidt, M.; Bender, R.; Riffeser, A. +4 more

We explore several ways to dissect brightest cluster galaxies (BCGs) and their surrounding intracluster light (ICL) using a surface brightness (SB) cut, a luminosity cut, excess light above a de Vaucouleurs profile, or a double Sérsic decomposition. Assuming that all light above $M\lt -21.85\,g^{\prime} \ \mathrm{mag}$ is attributable to the ICL, …

2021 The Astrophysical Journal Supplement Series
eHST 52
TESS Hunt for Young and Maturing Exoplanets (THYME). V. A Sub-Neptune Transiting a Young Star in a Newly Discovered 250 Myr Association
DOI: 10.3847/1538-3881/abdf53 Bibcode: 2021AJ....161..171T

Vanderburg, Andrew; Latham, David W.; Quinn, Samuel N. +27 more

The detection and characterization of young planetary systems offer a direct path to study the processes that shape planet evolution. We report on the discovery of a sub-Neptune-sized planet orbiting the young star HD 110082 (TOI-1098). Transit events we initially detected during TESS Cycle 1 are validated with time-series photometry from Spitzer.…

2021 The Astronomical Journal
Gaia 52
Local spiral structure based on the Gaia EDR3 parallaxes
DOI: 10.1051/0004-6361/202040103 Bibcode: 2021A&A...645L...8X

Hao, C. J.; Xu, Y.; Hou, L. G. +4 more

Context. The astrometric satellite Gaia is expected to significantly increase our knowledge as to the properties of the Milky Way. The Gaia Early Data Release 3 (EDR3) provides the most precise parallaxes for many OB stars, which can be used to delineate the Galactic spiral structure.
Aims: We investigate the local spiral structure with the l…

2021 Astronomy and Astrophysics
Gaia 52
Quantifying Feedback from Narrow Line Region Outflows in Nearby Active Galaxies. III. Results for the Seyfert 2 Galaxies Markarian 3, Markarian 78, and NGC 1068
DOI: 10.3847/1538-4357/abdcad Bibcode: 2021ApJ...910..139R

Rafelski, Marc; Fischer, Travis C.; Collins, Nicholas R. +9 more

Outflows of ionized gas driven by active galactic nuclei (AGN) may significantly impact the evolution of their host galaxies. However, determining the energetics of these outflows is difficult with spatially unresolved observations that are subject to strong global selection effects. We present part of an ongoing study using Hubble Space Telescope…

2021 The Astrophysical Journal
eHST 52
An inventory of atomic species in the atmosphere of WASP-121b using UVES high-resolution spectroscopy
DOI: 10.1093/mnras/stab1878 Bibcode: 2021MNRAS.506.3853M

Nikolov, Nikolay; de Mooij, Ernst J. W.; Gibson, Neale P. +8 more

Ultrahot Jupiters (UHJs) present excellent targets for atmospheric characterization. Their hot dayside temperatures (T ≳ 2200 K) strongly suppress the formation of condensates, leading to clear and highly inflated atmospheres extremely conducive to transmission spectroscopy. Recent studies using optical high-resolution spectra have discovered a pl…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 52
Gaia EDR3 Parallax Zero-point Offset Based on W Ursae Majoris-type Eclipsing Binaries
DOI: 10.3847/2041-8213/abf359 Bibcode: 2021ApJ...911L..20R

Huang, Yang; Deng, Licai; de Grijs, Richard +3 more

We independently determine the zero-point offset of the Gaia early Data Release-3 (EDR3) parallaxes based on ∼110,000 W Ursae Majoris (EW)-type eclipsing binary systems. EWs cover almost the entire sky and are characterized by a relatively complete coverage in magnitude and color. They are an excellent proxy for Galactic main-sequence stars. We de…

2021 The Astrophysical Journal
Gaia 52