Search Publications

The discovery of rest-frame UV colour gradients and a diversity of dust morphologies in bright z ≃ 7 Lyman-break galaxies
DOI: 10.1093/mnras/stab3744 Bibcode: 2022MNRAS.510.5088B

Bowler, R. A. A.; Cullen, F.; McLure, R. J. +2 more

We present deep ALMA dust continuum observations for a sample of luminous (MUV < -22) star-forming galaxies at z ≃ 7. We detect five of the six sources in the far-infrared (FIR), providing key constraints on the obscured star formation rate (SFR) and the infrared-excess-β (IRX-β) relation without the need for stacking. Despite the ga…

2022 Monthly Notices of the Royal Astronomical Society
eHST 50
NGC 5846-UDG1: A Galaxy Formed Mostly by Star Formation in Massive, Extremely Dense Clumps of Gas
DOI: 10.3847/2041-8213/ac590a Bibcode: 2022ApJ...927L..28D

van Dokkum, Pieter; Romanowsky, Aaron J.; Conroy, Charlie +10 more

It has been shown that ultra-diffuse galaxies (UDGs) have higher specific frequencies of globular clusters, on average, than other dwarf galaxies with similar luminosities. The UDG NGC 5846-UDG1 is among the most extreme examples of globular cluster-rich galaxies found so far. Here we present new Hubble Space Telescope observations and analysis of…

2022 The Astrophysical Journal
eHST 50
Fast plasmoid-mediated reconnection in a solar flare
DOI: 10.1038/s41467-022-28269-w Bibcode: 2022NatCo..13..640Y

Feng, Xueshang; Song, Yongliang; Xue, Zhike +8 more

Magnetic reconnection is a multi-faceted process of energy conversion in astrophysical, space and laboratory plasmas that operates at microscopic scales but has macroscopic drivers and consequences. Solar flares present a key laboratory for its study, leaving imprints of the microscopic physics in radiation spectra and allowing the macroscopic evo…

2022 Nature Communications
Hinode 50
Sizes of Lensed Lower-luminosity z = 4-8 Galaxies from the Hubble Frontier Field Program
DOI: 10.3847/1538-4357/ac4791 Bibcode: 2022ApJ...927...81B

Oesch, P. A.; Bouwens, R. J.; Illingworth, G. D. +3 more

We constrain the rest-UV size-luminosity relation for star-forming galaxies at z ~ 4 and z ~ 6, 7, and 8 identified behind clusters from the Hubble Frontier Fields (HFF) program. The size-luminosity relation is key to deriving accurate luminosity functions (LF) for faint galaxies. Making use of the latest lensing models and full data set for these…

2022 The Astrophysical Journal
eHST 49
Determination of X-ray pulsar geometry with IXPE polarimetry
DOI: 10.1038/s41550-022-01799-5 Bibcode: 2022NatAs...6.1433D

Wu, Kinwah; Enoto, Teruaki; Turolla, Roberto +91 more

Using observations of X-ray pulsar Hercules X-1 by the Imaging X-ray Polarimetry Explorer we report a highly significant (>17σ) detection of the polarization signal from an accreting neutron star. The observed degree of linear polarization of ~10% is far below theoretical expectations for this object, and stays low throughout the spin cycle of …

2022 Nature Astronomy
Gaia 49
Implications for galaxy formation models from observations of globular clusters around ultra-diffuse galaxies
DOI: 10.1093/mnras/stac328 Bibcode: 2022MNRAS.511.4633S

Beasley, Michael A.; Trujillo, Ignacio; Peletier, Reynier F. +5 more

We present an analysis of Hubble Space Telescope observations of globular clusters (GCs) in six ultradiffuse galaxies (UDGs) in the Coma cluster, a sample that represents UDGs with large effective radii (Re), and use the results to evaluate competing formation models. We eliminate two significant sources of systematic uncertainty in the…

2022 Monthly Notices of the Royal Astronomical Society
eHST 49
Planetary Nebulae: Sources of Enlightenment
DOI: 10.1088/1538-3873/ac32b1 Bibcode: 2022PASP..134b2001K

Henry, R. B. C.; Kwitter, Karen B.

In this review/tutorial we explore planetary nebulae as a stage in the evolution of low-to-intermediate-mass stars, as major contributors to the mass and chemical enrichment of the interstellar medium, and as astrophysical laboratories. We discuss many observed properties of planetary nebulae, placing particular emphasis on element abundance deter…

2022 Publications of the Astronomical Society of the Pacific
Gaia 49
The X-shooter Spectral Library (XSL): Data Release 3
DOI: 10.1051/0004-6361/202142388 Bibcode: 2022A&A...660A..34V

Peletier, R. F.; Arentsen, A.; Coelho, P. R. T. +12 more

We present the third data release (DR3) of the X-shooter Spectral Library (XSL). This moderate-to-high resolution, near-ultraviolet-to-near-infrared (350-2480 nm, R ∼ 10 000) spectral library is composed of 830 stellar spectra of 683 stars. DR3 improves upon the previous data release by providing the combined de-reddened spectra of the three X-sho…

2022 Astronomy and Astrophysics
Gaia eHST 49
High Equivalent Width of Hα+[N II] Emission in z 8 Lyman-break Galaxies from IRAC 5.8 µm Observations: Evidence for Efficient Lyman-continuum Photon Production in the Epoch of Reionization
DOI: 10.3847/1538-4357/ac7e44 Bibcode: 2022ApJ...935...94S

Illingworth, Garth D.; Labbé, Ivo; Bouwens, Rychard J. +3 more

We measure, for the first time, the median equivalent width (EW) of Hα+[N II] in star-forming galaxies at z ~ 8. Our estimate leverages the unique photometric depth of the Spitzer/IRAC 5.8 µm band mosaics (probing ≈5500-7100 Å at z ~ 8) of the GOODS Reionization Era Wide Area Treasury from Spitzer (GREATS) program. We median-stacked the stam…

2022 The Astrophysical Journal
eHST 49
MHD disc winds can reproduce fast disc dispersal and the correlation between accretion rate and disc mass in Lupus
DOI: 10.1093/mnrasl/slab124 Bibcode: 2022MNRAS.512L..74T

Lodato, G.; van Dishoeck, E. F.; Tabone, B. +3 more

The final architecture of planetary systems depends on the extraction of angular momentum and mass-loss processes of the discs in which they form. Theoretical studies proposed that magnetohydrodynamic winds launched from the discs (MHD disc winds) could govern accretion and disc dispersal. In this work, we revisit the observed disc demographics in…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 49