Search Publications

On the inconsistency of [C/Fe] abundances and the fractions of carbon-enhanced metal-poor stars among various stellar surveys
DOI: 10.1093/mnras/stac2062 Bibcode: 2022MNRAS.515.4082A

Yoon, Jinmi; Lee, Young Sun; Placco, Vinicius M. +4 more

Carbon-enhanced metal-poor (CEMP) stars are a unique resource for Galactic archaeology because they probe the properties of the First Stars, early chemical evolution, and binary interactions at very low metallicity. Comparing the fractions and properties of CEMP stars in different Galactic environments can provide us with unique insights into the …

2022 Monthly Notices of the Royal Astronomical Society
Gaia 33
The primordial matter power spectrum on sub-galactic scales
DOI: 10.1093/mnras/stac670 Bibcode: 2022MNRAS.512.3163G

Treu, Tommaso; Bovy, Jo; Birrer, Simon +3 more

The primordial matter power spectrum quantifies fluctuations in the distribution of dark matter immediately following inflation. Over cosmic time, overdense regions of the primordial density field grow and collapse into dark matter haloes, whose abundance and density profiles retain memory of the initial conditions. By analysing the image magnific…

2022 Monthly Notices of the Royal Astronomical Society
eHST 33
Magnetic braking saturates: evidence from the orbital period distribution of low-mass detached eclipsing binaries from ZTF
DOI: 10.1093/mnras/stac2945 Bibcode: 2022MNRAS.517.4916E

Conroy, Charlie; Kiman, Rocio; El-Badry, Kareem +4 more

We constrain the orbital period (Porb) distribution of low-mass detached main-sequence eclipsing binaries (EBs) with light-curves from the Zwicky Transient Facility (ZTF), which provides a well-understood selection function and sensitivity to faint stars. At short periods (Porb ≲ 2 d), binaries are predicted to evolve signifi…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 33
The Pristine dwarf galaxy survey - IV. Probing the outskirts of the dwarf galaxy Boötes I
DOI: 10.1093/mnras/stac1827 Bibcode: 2022MNRAS.516.2348L

Sestito, Federico; McConnachie, Alan W.; Navarro, Julio F. +12 more

We present a new spectroscopic study of the dwarf galaxy Boötes I (Boo I) with data from the Anglo-Australian Telescope and its AAOmega spectrograph together with the Two Degree Field multi-object system. We observed 36 high-probability Boo I stars selected using Gaia Early Data Release 3 proper motions and photometric metallicities from the Prist…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 32
Internal kinematics of Gaia eDR3 wide binaries
DOI: 10.1093/mnras/stab3038 Bibcode: 2022MNRAS.509.2304H

Hernandez, X.; Cortés, R. A. M.; Cookson, S.

Using the recent Gaia eDR3 catalogue, we construct a sample of solar neighbourhood isolated wide binaries satisfying a series of strict signal-to-noise data cuts, exclusion of random association criteria, and detailed colour-magnitude diagram selections to minimize the presence of any kinematic contaminating effects having been discussed in the li…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 32
How much hydrogen is in Type Ib and IIb supernova progenitors?
DOI: 10.1093/mnras/stac088 Bibcode: 2022MNRAS.511..691G

Arcavi, Iair; Gilkis, Avishai

Core-collapse supernovae showing little or no hydrogen (denoted by Type IIb and Ib, respectively) are the explosions of massive stars that have lost some or most of their outer envelopes. How they lose their mass is unclear, but it likely involves binary interaction. So far, seven progenitors of such supernovae have been identified in pre-explosio…

2022 Monthly Notices of the Royal Astronomical Society
eHST 32
Exploring the dependence of hot Jupiter occurrence rates on stellar mass with TESS
DOI: 10.1093/mnras/stac2179 Bibcode: 2022MNRAS.516...75B

Kunimoto, M.; Beleznay, Maya

We present estimates for the occurrence rates of hot Jupiters around dwarf stars based on data from the Transiting Exoplanet Survey Satellite (TESS) Prime Mission. We take 97 hot Jupiters orbiting 198 721 AFG dwarf stars (ranging in mass from 0.8 to $2.3\, {\rm M}_{\odot }$) from an independent search for hot Jupiters using TESS Prime Mission data…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 32
INTEGRAL/IBIS 17-yr hard X-ray all-sky survey
DOI: 10.1093/mnras/stab3751 Bibcode: 2022MNRAS.510.4796K

Tsygankov, Sergey S.; Lutovinov, Alexander A.; Krivonos, Roman A. +3 more

The International Gamma-Ray Astrophysics Laboratory (INTEGRAL), launched in 2002, continues its successful work in observing the sky at energies E > 20 keV. The legacy of the mission already includes a large number of discovered or previously poorly studied hard X-ray sources. The growing INTEGRAL archive allows one to conduct an all-sky survey…

2022 Monthly Notices of the Royal Astronomical Society
INTEGRAL XMM-Newton 31
Radio and far-IR emission associated with a massive star-forming galaxy candidate at z ≃ 6.8: a radio-loud AGN in the reionization era?
DOI: 10.1093/mnras/stac737 Bibcode: 2022MNRAS.512.4248E

Fan, Xiaohui; Stark, Daniel P.; Endsley, Ryan +7 more

We report the identification of radio (0.144-3 GHz) and mid-, far-infrared, and sub-mm (24-850µm) emission at the position of one of 41 UV-bright ($\mathrm{M_{\mathrm{UV}}}^{ }\lesssim -21.25$) z ≃ 6.6-6.9 Lyman-break galaxy candidates in the 1.5 deg2 COSMOS field. This source, COS-87259, exhibits a sharp flux discontinuity (facto…

2022 Monthly Notices of the Royal Astronomical Society
Herschel eHST 31
The Cosmic Ultraviolet Baryon Survey (CUBS) V: on the thermodynamic properties of the cool circumgalactic medium at z ≲ 1
DOI: 10.1093/mnras/stac2528 Bibcode: 2022MNRAS.516.4882Q

Faucher-Giguère, Claude-André; Johnson, Sean D.; Zahedy, Fakhri S. +11 more

This paper presents a systematic study of the photoionization and thermodynamic properties of the cool circumgalactic medium (CGM) as traced by rest-frame ultraviolet absorption lines around 26 galaxies at redshift z ≲ 1. The study utilizes both high-quality far-ultraviolet and optical spectra of background QSOs and deep galaxy redshift surveys to…

2022 Monthly Notices of the Royal Astronomical Society
eHST 31