Search Publications

The recurrent impact of the Sagittarius dwarf on the star formation history of the Milky Way
DOI: 10.1038/s41550-020-1097-0 Bibcode: 2020NatAs...4..965R

Ruiz-Lara, Tomás; Bernard, Edouard J.; Cassisi, Santi +1 more

Satellites orbiting disk galaxies can induce phase space features such as spirality, vertical heating and phase-mixing in their disks. Such features have also been observed in our own Galaxy, but the complexity of the Milky Way disk has only recently been fully mapped by Gaia Data Release 2 (DR2) data. This complex behaviour is mainly ascribed to …

2020 Nature Astronomy
Gaia 142
Resonance locking in giant planets indicated by the rapid orbital expansion of Titan
DOI: 10.1038/s41550-020-1120-5 Bibcode: 2020NatAs...4.1053L

Fuller, Jim; Modenini, Dario; Tortora, Paolo +8 more

Saturn is orbited by dozens of moons, and the intricate dynamics of this complex system provide clues about its formation and evolution. Tidal friction within Saturn causes its moons to migrate outwards, driving them into orbital resonances that pump their eccentricities or inclinations, which in turn leads to tidal heating of the moons. However, …

2020 Nature Astronomy
eHST 112
Evidence of ammonium salts in comet 67P as explanation for the nitrogen depletion in cometary comae
DOI: 10.1038/s41550-019-0991-9 Bibcode: 2020NatAs...4..533A

De Keyser, Johan; Gombosi, Tamas I.; Berthelier, Jean-Jacques +14 more

Cometary comae are generally depleted in nitrogen. The main carriers for volatile nitrogen in comets are NH3 and HCN. It is known that ammonia readily combines with many acids, such as HCN, HNCO and HCOOH, encountered in the interstellar medium as well as in cometary ice to form ammonium salts (NH4+X-) a…

2020 Nature Astronomy
Rosetta 109
Coherent radio emission from a quiescent red dwarf indicative of star-planet interaction
DOI: 10.1038/s41550-020-1011-9 Bibcode: 2020NatAs...4..577V

White, G. J.; Callingham, J. R.; Shimwell, T. W. +11 more

Low-frequency (ν ≲ 150 MHz) stellar radio emission is expected to originate in the outer corona at heights comparable to and larger than the stellar radius. Such emission from the Sun has been used to study coronal structure, mass ejections and space-weather conditions around the planets1. Searches for low-frequency emission from other …

2020 Nature Astronomy
Gaia 107
A dynamic black hole corona in an active galaxy through X-ray reverberation mapping
DOI: 10.1038/s41550-019-1002-x Bibcode: 2020NatAs...4..597A

Fabian, Andrew C.; Middleton, Matthew J.; Walton, Dominic J. +18 more

X-ray reverberation echoes are assumed to be produced in the strongly distorted spacetime around accreting supermassive black holes. This signal allows us to spatially map the geometry of the inner accretion flow1,2—a region that cannot yet be spatially resolved by any telescope—and provides a direct measure of the black hole mass and s…

2020 Nature Astronomy
XMM-Newton 88
A kilonova associated with GRB 070809
DOI: 10.1038/s41550-019-0892-y Bibcode: 2020NatAs...4...77J

Li, Xiang; Jin, Zhi-Ping; Covino, Stefano +4 more

For on-axis typical short gamma-ray bursts (sGRBs), the forward shock emission is usually so bright1,2 that it renders the identification of kilonovae (also known as macronovae)3-6 in the early afterglow (t < 0.5 d) phase rather challenging. This is why previously no thermal-like kilonova component has been identified at s…

2020 Nature Astronomy
eHST 79
Direct evidence for shock-powered optical emission in a nova
DOI: 10.1038/s41550-020-1070-y Bibcode: 2020NatAs...4..776A

Wade, Gregg A.; Moffat, Anthony F. J.; Izzo, Luca +39 more

Classical novae are thermonuclear explosions that occur on the surfaces of white dwarf stars in interacting binary systems1. It has long been thought that the luminosity of classical novae is powered by continued nuclear burning on the surface of the white dwarf after the initial runaway2. However, recent observations of giga…

2020 Nature Astronomy
XMM-Newton 79
A heatwave of accretion energy traced by masers in the G358-MM1 high-mass protostar
DOI: 10.1038/s41550-019-0989-3 Bibcode: 2020NatAs...4..506B

Eislöffel, J.; Stecklum, B.; Kim, Kee-Tae +20 more

High-mass stars are thought to accumulate much of their mass via short, infrequent bursts of disk-aided accretion1,2. Such accretion events are rare and difficult to observe directly but are known to drive enhanced maser emission3-6. In this Letter we report high-resolution, multi-epoch methanol maser observations toward G358…

2020 Nature Astronomy
Gaia 78
Evidence for a vast prograde stellar stream in the solar vicinity
DOI: 10.1038/s41550-020-1131-2 Bibcode: 2020NatAs...4.1078N

Hopkins, Philip F.; Sanderson, Robyn; Wetzel, Andrew +6 more

Massive dwarf galaxies that merge with the Milky Way on prograde orbits can be dragged into the disk plane before being completely disrupted. Such mergers can contribute to an accreted stellar disk and a dark matter disk. Here we present Nyx, a vast stellar stream in the vicinity of the Sun, which provides the first indication that such an event o…

2020 Nature Astronomy
Gaia 74
The carbon monoxide-rich interstellar comet 2I/Borisov
DOI: 10.1038/s41550-020-1095-2 Bibcode: 2020NatAs...4..867B

Feldman, P. D.; Bodewits, D.; Noonan, J. W. +7 more

Interstellar comets offer direct samples of volatiles from distant protoplanetary disks. 2I/Borisov is the first notably active interstellar comet discovered in our Solar System1. Comets are condensed samples of the gas, ice and dust that were in a star's protoplanetary disk during the formation of its planets, and inform our understand…

2020 Nature Astronomy
eHST 74