Search Publications

Coronal Mass Ejections over Solar Cycles 23 and 24
DOI: 10.1007/s11214-019-0605-y Bibcode: 2019SSRv..215...39L

Lamy, P. L.; Gilardy, H.; Floyd, O. +3 more

We present a statistical analysis of solar coronal mass ejections (CMEs) based on 23 years of quasi-continuous observations with the LASCO coronagraph, thus covering two complete Solar Cycles (23 and 24). We make use of five catalogs, one manual (CDAW) and four automated (ARTEMIS, CACTus, SEEDS, and CORIMP), to characterize the temporal evolutions…

2019 Space Science Reviews
SOHO 95
Observation-based modelling of magnetised coronal mass ejections with EUHFORIA
DOI: 10.1051/0004-6361/201935053 Bibcode: 2019A&A...626A.122S

Mierla, M.; Rodriguez, L.; Poedts, S. +2 more

Context. Coronal mass ejections (CMEs) are the primary source of strong space weather disturbances at Earth. Their geo-effectiveness is largely determined by their dynamic pressure and internal magnetic fields, for which reliable predictions at Earth are not possible with traditional cone CME models.
Aims: We study two well-observed Earth-dir…

2019 Astronomy and Astrophysics
SOHO 95
TESS Spots a Compact System of Super-Earths around the Naked-eye Star HR 858
DOI: 10.3847/2041-8213/ab322d Bibcode: 2019ApJ...881L..19V

Vanderburg, Andrew; Bieryla, Allyson; Latham, David W. +48 more

Transiting Exoplanet Survey Satellite (TESS) observations have revealed a compact multiplanet system around the sixth-magnitude star HR 858 (TIC 178155732, TOI 396), located 32 pc away. Three planets, each about twice the size of Earth, transit this slightly evolved, late F-type star, which is also a member of a visual binary. Two of the planets m…

2019 The Astrophysical Journal
Gaia 94
Extended stellar systems in the solar neighborhood. I. The tidal tails of the Hyades
DOI: 10.1051/0004-6361/201834622 Bibcode: 2019A&A...621L...3M

Meingast, Stefan; Alves, João

We report the discovery of two well-defined tidal tails emerging from the Hyades star cluster. The tails were detected in Gaia DR2 data by selecting cluster members in the 3D galactocentric cylindrical velocity space. The robustness of our member selection is reinforced by the fact that the sources depict an almost noiseless, coeval stellar main s…

2019 Astronomy and Astrophysics
Gaia 94
Space Densities and Emissivities of Active Galactic Nuclei at z > 4
DOI: 10.3847/1538-4357/ab39e1 Bibcode: 2019ApJ...884...19G

Dickinson, M.; Fiore, F.; Castellano, M. +11 more

The study of the space density of bright active galactic nuclei (AGNs) at z > 4 has been subject to extensive effort given its importance in the estimation of cosmological ionizing emissivity and growth of supermassive black holes. In this context we have recently derived high space densities of AGNs at z ∼ 4 and -25 < M 1450 <…

2019 The Astrophysical Journal
eHST 93
The East Asian Observatory SCUBA-2 Survey of the COSMOS Field: Unveiling 1147 Bright Sub-millimeter Sources across 2.6 Square Degrees
DOI: 10.3847/1538-4357/ab23ff Bibcode: 2019ApJ...880...43S

Thomson, A. P.; Ivison, R. J.; Smail, Ian +28 more

We present sensitive 850 µm imaging of the Cosmological Evolution Survey (COSMOS) field using 640 hr of new and archival observations taken with SCUBA-2 at the East Asian Observatory’s James Clerk Maxwell Telescope. The SCUBA-2 COSMOS survey (S2COSMOS) achieves a median noise level of σ 850µm = 1.2 mJy beam-1 over…

2019 The Astrophysical Journal
Herschel 93
The Ophiuchus DIsk Survey Employing ALMA (ODISEA): Disk Dust Mass Distributions across Protostellar Evolutionary Classes
DOI: 10.3847/2041-8213/ab1338 Bibcode: 2019ApJ...875L...9W

Ansdell, Megan; Williams, Jonathan P.; Casassus, Simon +5 more

As protostars evolve from optically faint/infrared-bright (Class I) sources to optically bright/infrared-faint (Class II) the solid material in their surrounding disks accumulates into planetesimals and protoplanets. The nearby, young Ophiuchus star-forming region contains hundreds of protostars in a range of evolutionary states. Using the Atacama…

2019 The Astrophysical Journal
Gaia 93
The FMOS-COSMOS Survey of Star-forming Galaxies at z ∼ 1.6. VI. Redshift and Emission-line Catalog and Basic Properties of Star-forming Galaxies
DOI: 10.3847/1538-4365/ab06c4 Bibcode: 2019ApJS..241...10K

Koekemoer, Anton M.; Daddi, Emanuele; Juneau, Stéphanie +12 more

We present a new data release from the Fiber Multi-Object Spectrograph (FMOS)-COSMOS survey that contains the measurements of the spectroscopic redshift and flux of rest-frame optical emission lines (Hα, [N II], [S II], Hβ, [O III]) for 1931 galaxies out of a total of 5484 objects observed over the 1.7 deg2 COSMOS field. We obtained H- …

2019 The Astrophysical Journal Supplement Series
Herschel 93
Black hole masses of tidal disruption event host galaxies II
DOI: 10.1093/mnras/stz1602 Bibcode: 2019MNRAS.487.4136W

Jonker, Peter G.; Stone, Nicholas C.; Auchettl, Katie +8 more

We present new medium resolution, optical long-slit spectra of a sample of six ultraviolet (UV)/optical and 17 X-ray-selected tidal disruption event candidate host galaxies. We measure emission line ratios from the optical spectra, finding that the large majority of hosts are quiescent galaxies, while those displaying emission lines are generally …

2019 Monthly Notices of the Royal Astronomical Society
XMM-Newton 93
Age Determination in Upper Scorpius with Eclipsing Binaries
DOI: 10.3847/1538-4357/aafe09 Bibcode: 2019ApJ...872..161D

Howell, Steve B.; Isaacson, Howard T.; Livingston, John H. +4 more

The Upper Scorpius OB association is the nearest region of recent massive star formation and thus an important benchmark for investigations concerning stellar evolution and planet formation timescales. We present nine eclipsing binaries (EBs) in Upper Scorpius, three of which are newly reported here and all of which were discovered from K2 photome…

2019 The Astrophysical Journal
Gaia 93