Search Publications

An ultra-massive white dwarf with a mixed hydrogen-carbon atmosphere as a likely merger remnant
DOI: 10.1038/s41550-020-1028-0 Bibcode: 2020NatAs...4..663H

Gänsicke, B. T.; Dhillon, V. S.; Tremblay, P. -E. +11 more

White dwarfs are dense, cooling stellar embers consisting mostly of carbon and oxygen1, or oxygen and neon (with a few per cent carbon) at higher initial stellar masses2. These stellar cores are enveloped by a shell of helium, which in turn, is usually surrounded by a layer of hydrogen, generally prohibiting direct observatio…

2020 Nature Astronomy
Gaia 42
AstroSat detection of Lyman continuum emission from a z = 1.42 galaxy
DOI: 10.1038/s41550-020-1173-5 Bibcode: 2020NatAs...4.1185S

Verhamme, Anne; Inoue, Akio K.; Schaerer, Daniel +10 more

One of the outstanding problems of current observational cosmology is to understand the nature of sources that produced the bulk of the ionizing radiation after the Cosmic Dark Age. Direct detection of these reionization sources1 is practically infeasible at high redshift (z) due to the steep decline of intergalactic medium transmission…

2020 Nature Astronomy
eHST 40
Common dynamo scaling in slowly rotating young and evolved stars
DOI: 10.1038/s41550-020-1039-x Bibcode: 2020NatAs...4..658L

Spada, Federico; Lehtinen, Jyri J.; Käpylä, Maarit J. +2 more

One interpretation of the activity and magnetism of late-type stars is that these both intensify with decreasing Rossby number up to a saturation level1-3, suggesting that stellar dynamos depend on both rotation and convective turbulence4. Some studies have claimed, however, that rotation alone suffices to parametrize this sc…

2020 Nature Astronomy
Gaia 38
Resolving the Crab pulsar wind nebula at teraelectronvolt energies
DOI: 10.1038/s41550-019-0910-0 Bibcode: 2020NatAs...4..167H

H. E. S. S. Collaboration

The Crab nebula is one of the most-studied cosmic particle accelerators, shining brightly across the entire electromagnetic spectrum up to very-high-energy gamma rays1,2. It is known from observations in the radio to gamma-ray part of the spectrum that the nebula is powered by a pulsar, which converts most of its rotational energy losse…

2020 Nature Astronomy
XMM-Newton 35
A basin-free spherical shape as an outcome of a giant impact on asteroid Hygiea
DOI: 10.1038/s41550-019-0915-8 Bibcode: 2020NatAs...4..136V

Jorda, L.; Lamy, P.; Colas, F. +44 more

(10) Hygiea is the fourth largest main belt asteroid and the only known asteroid whose surface composition appears similar to that of the dwarf planet (1) Ceres1,2, suggesting a similar origin for these two objects. Hygiea suffered a giant impact more than 2 Gyr ago3 that is at the origin of one of the largest asteroid famili…

2020 Nature Astronomy
AKARI 34
An eclipsing substellar binary in a young triple system discovered by SPECULOOS
DOI: 10.1038/s41550-020-1018-2 Bibcode: 2020NatAs...4..650T

Kunovac Hodžić, Vedad; Triaud, Amaury H. M. J.; Burgasser, Adam J. +18 more

Mass, radius and age are three of the most fundamental parameters for celestial objects, enabling insight into the evolution and internal physics of stars, brown dwarfs and planets. Brown dwarfs are hydrogen-rich objects that are unable to sustain core fusion reactions but are supported against collapse by electron degeneracy pressure1.…

2020 Nature Astronomy
Gaia 34
Global helium abundance measurements in the solar corona
DOI: 10.1038/s41550-020-1156-6 Bibcode: 2020NatAs...4.1134M

Telloni, Daniele; Antonucci, Ester; Fineschi, Silvano +24 more

Solar abundances have been historically assumed to be representative of cosmic abundances. However, our knowledge of the solar abundance of helium, the second most abundant element, relies mainly on models1 and indirect measurements through helioseismic observations2, because actual measurements of helium in the solar atmosph…

2020 Nature Astronomy
SOHO 30
A pulsating white dwarf in an eclipsing binary
DOI: 10.1038/s41550-020-1037-z Bibcode: 2020NatAs...4..690P

Hermes, J. J.; Parsons, Steven G.; Breedt, Elmé +8 more

White dwarfs are the burnt-out cores of Sun-like stars and are the fate of 97 per cent of the stars in our Galaxy. The internal structure and composition of white dwarfs are hidden by their high gravities, which causes all elements apart from the lightest ones to settle out of their atmospheres. The most direct method of probing the inner structur…

2020 Nature Astronomy
Gaia 26
Infalling gas in a Lyman-α blob
DOI: 10.1038/s41550-020-1033-3 Bibcode: 2020NatAs...4..670A

Kohno, Kotaro; Lehnert, Matthew D.; Menten, Karl M. +11 more

Lyman-α blobs (LABs) are spatially extended nebulae of emission in the Lyman-α (Lyα) line of hydrogen, seen at high redshifts1,2, and most commonly found in the dense environment of star-forming galaxies3,4. A recent study showed that nearly 100% of the sky is covered by Lyα emission around high-redshift galaxies5-7

2020 Nature Astronomy
Herschel 26
Highlights of exoplanetary science from Spitzer
DOI: 10.1038/s41550-020-1100-9 Bibcode: 2020NatAs...4..453D

Deming, Drake; Knutson, Heather A.

Observations of extrasolar planets were not projected to be a substantial part of the Spitzer Space Telescope's mission when it was conceived and designed. Nevertheless, Spitzer was the first facility to detect thermal emission from a hot Jupiter-sized planet, and the range of its exoplanetary investigations grew to encompass transiting planets, m…

2020 Nature Astronomy
eHST 24