Search Publications

Observational constraints on dust disk sizes in tidally truncated protoplanetary disks in multiple systems in the Taurus region
DOI: 10.1051/0004-6361/201935964 Bibcode: 2019A&A...628A..95M

Liu, Y.; Lodato, G.; van der Plas, G. +16 more

The impact of stellar multiplicity on the evolution of planet-forming disks is still the subject of debate. Here we present and analyze disk structures around ten multiple stellar systems that were included in an unbiased, high spatial resolution survey performed with ALMA of 32 protoplanetary disks in the Taurus star-forming region. At the unprec…

2019 Astronomy and Astrophysics
Gaia 92
Kinematics of the Broad-line Region of 3C 273 from a 10 yr Reverberation Mapping Campaign
DOI: 10.3847/1538-4357/ab1099 Bibcode: 2019ApJ...876...49Z

Ho, Luis C.; Smith, Paul S.; Zhang, Zhi-Xiang +9 more

Despite many decades of study, the kinematics of the broad-line region of 3C 273 are still poorly understood. We report a new, high signal-to-noise, reverberation mapping campaign carried out from 2008 November to 2018 March that allows the determination of time lags between emission lines and the variable continuum with high precision. The time l…

2019 The Astrophysical Journal
eHST 92
Sunyaev-Zel'dovich effect and X-ray scaling relations from weak lensing mass calibration of 32 South Pole Telescope selected galaxy clusters
DOI: 10.1093/mnras/sty3088 Bibcode: 2019MNRAS.483.2871D

Bayliss, M. B.; Schrabback, T.; von der Linden, A. +28 more

Uncertainty in mass-observable scaling relations is currently the limiting factor for galaxy-cluster-based cosmology. Weak gravitational lensing can provide direct mass calibration and reduce the mass uncertainty. We present new ground-based weak lensing observations of 19 South Pole Telescope (SPT) selected clusters at redshifts 0.29 ≤ z ≤ 0.61 a…

2019 Monthly Notices of the Royal Astronomical Society
eHST 92
A 100-kiloparsec wind feeding the circumgalactic medium of a massive compact galaxy
DOI: 10.1038/s41586-019-1686-1 Bibcode: 2019Natur.574..643R

Coil, Alison; Moustakas, John; Diamond-Stanic, Aleksandar M. +9 more

Ninety per cent of baryons are located outside galaxies, either in the circumgalactic or intergalactic medium1,2. Theory points to galactic winds as the primary source of the enriched and massive circumgalactic medium3-6. Winds from compact starbursts have been observed to flow to distances somewhat greater than ten kiloparse…

2019 Nature
eHST 92
Explosive Magnetotail Activity
DOI: 10.1007/s11214-019-0599-5 Bibcode: 2019SSRv..215...31S

Khotyaintsev, Yuri; Velli, Marco; Runov, Andrei +13 more

Modes and manifestations of the explosive activity in the Earth's magnetotail, as well as its onset mechanisms and key pre-onset conditions are reviewed. Two mechanisms for the generation of the pre-onset current sheet are discussed, namely magnetic flux addition to the tail lobes, or other high-latitude perturbations, and magnetic flux evacuation…

2019 Space Science Reviews
Cluster 92
The magnetic early B-type stars - III. A main-sequence magnetic, rotational, and magnetospheric biography
DOI: 10.1093/mnras/stz2551 Bibcode: 2019MNRAS.490..274S

Wade, G. A.; Neiner, C.; Shultz, M. E. +10 more

Magnetic confinement of stellar winds leads to the formation of magnetospheres, which can be sculpted into centrifugal magnetospheres (CMs) by rotational support of the corotating plasma. The conditions required for the CMs of magnetic early B-type stars to yield detectable emission in H α - the principal diagnostic of these structures - are poorl…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 92
Dynamics of cluster-forming hub-filament systems. The case of the high-mass star-forming complex Monoceros R2
DOI: 10.1051/0004-6361/201935260 Bibcode: 2019A&A...629A..81T

Schneider, N.; Tremblin, P.; Didelon, P. +15 more

Context. High-mass stars and star clusters commonly form within hub-filament systems. Monoceros R2 (hereafter Mon R2), at a distance of 830 pc, harbors one of the closest of these systems, making it an excellent target for case studies.
Aims: We investigate the morphology, stability and dynamical properties of the Mon R2 hub-filament system. …

2019 Astronomy and Astrophysics
Herschel 91
A Hot Saturn Orbiting an Oscillating Late Subgiant Discovered by TESS
DOI: 10.3847/1538-3881/ab1488 Bibcode: 2019AJ....157..245H

Henning, Thomas; Smalley, Barry; Chaplin, William J. +139 more

We present the discovery of HD 221416 b, the first transiting planet identified by the Transiting Exoplanet Survey Satellite (TESS) for which asteroseismology of the host star is possible. HD 221416 b (HIP 116158, TOI-197) is a bright (V = 8.2 mag), spectroscopically classified subgiant that oscillates with an average frequency of about 430 µ…

2019 The Astronomical Journal
Gaia 91
A public relativistic transfer function model for X-ray reverberation mapping of accreting black holes
DOI: 10.1093/mnras/stz1720 Bibcode: 2019MNRAS.488..324I

Ingram, Adam; García, Javier A.; Mastroserio, Guglielmo +3 more

We present the publicly available model RELTRANS that calculates the light-crossing delays and energy shifts experienced by X-ray photons originally emitted close to the black hole when they reflect from the accretion disc and are scattered into our line of sight, accounting for all general relativistic effects. Our model is fast and flexible enou…

2019 Monthly Notices of the Royal Astronomical Society
XMM-Newton 91
Dynamical Confirmation of a Black Hole in MAXI J1820+070
DOI: 10.3847/2041-8213/ab39df Bibcode: 2019ApJ...882L..21T

Armas Padilla, M.; Jiménez-Ibarra, F.; Muñoz-Darias, T. +4 more

We present time-resolved 10.4 m Gran Telescopio Canarias and 4.2 m William Herschel Telescope intermediate resolution spectroscopy of the X-ray transient MAXI J1820+070 (=ASASSN-18ey) obtained during its decline to the quiescent state. Cross-correlation of the 21 individual spectra against late-type templates reveals a sinusoidal velocity modulati…

2019 The Astrophysical Journal
Gaia 91