Search Publications

The shape of the Galactic halo with Gaia DR2 RR Lyrae. Anatomy of an ancient major merger
DOI: 10.1093/mnras/sty2806 Bibcode: 2019MNRAS.482.3868I

Belokurov, Vasily; Iorio, Giuliano

We use the Gaia DR2 RR Lyrae sample to gain an uninterrupted view of the Galactic stellar halo. We dissect the available volume in slices parallel to the Milky Way's disc to show that within ∼30 kpc from the Galactic centre the halo is triaxial, with the longest axis misaligned by ∼70° with respect to the Galactic x-axis. This anatomical procedure…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 123
Potential kick velocity distribution of black hole X-ray binaries and implications for natal kicks
DOI: 10.1093/mnras/stz2335 Bibcode: 2019MNRAS.489.3116A

Maccarone, T. J.; Chaty, S.; Miller-Jones, J. C. A. +14 more

We use very long baseline interferometry to measure the proper motions of three black hole X-ray binaries (BHXBs). Using these results together with data from the literature and Gaia DR2 to collate the best available constraints on proper motion, parallax, distance, and systemic radial velocity of 16 BHXBs, we determined their three-dimensional Ga…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 122
ACCESS: a featureless optical transmission spectrum for WASP-19b from Magellan/IMACS
DOI: 10.1093/mnras/sty2691 Bibcode: 2019MNRAS.482.2065E

Fortney, Jonathan J.; López-Morales, Mercedes; Jordán, Andrés +13 more

The short-period (0.94-d) transiting exoplanet WASP-19b is an exceptional target for transmission spectroscopy studies, due to its relatively large atmospheric scale height (∼500 km) and equilibrium temperature (∼2100 K). Here, we report on six precise spectroscopic Magellan/IMACS observations, five of which target the full optical window from 0.4…

2019 Monthly Notices of the Royal Astronomical Society
eHST 121
The pattern speed of the Milky Way bar from transverse velocities
DOI: 10.1093/mnras/stz1827 Bibcode: 2019MNRAS.488.4552S

Evans, N. Wyn; Sanders, Jason L.; Smith, Leigh

We use the continuity equation to derive a method for measuring the pattern speed of the Milky Way's bar/bulge from proper motion data. The method has minimal assumptions but requires complete coverage of the non-axisymmetric component in two of the three Galactic coordinates. We apply our method to the proper motion data from a combination of Gai…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 121
The GREATS H β + [O III] luminosity function and galaxy properties at z ∼ 8: walking the way of JWST
DOI: 10.1093/mnras/stz940 Bibcode: 2019MNRAS.489.2355D

Oesch, P. A.; Bouwens, R. J.; Illingworth, G. D. +5 more

The James Webb Space Telescope will allow to spectroscopically study an unprecedented number of galaxies deep into the reionization era, notably by detecting [O III]λλ4959, 5007, and H β nebular emission lines. To efficiently prepare such observations, we photometrically select a large sample of galaxies at z ∼ 8 and study their rest-frame optical…

2019 Monthly Notices of the Royal Astronomical Society
eHST 120
Ingredients for solar-like systems: protostar IRAS 16293-2422 B versus comet 67P/Churyumov-Gerasimenko
DOI: 10.1093/mnras/stz2430 Bibcode: 2019MNRAS.490...50D

van Dishoeck, Ewine F.; Drozdovskaya, Maria N.; Jørgensen, Jes K. +2 more

Our modern day Solar System has 4.6 × 109 yr of evolution behind it with just a few relics of its birth conditions remaining. Comets are thought to be some of the most pristine tracers of the initial ingredients that were combined to produce the Earth and the other planets. Other low-mass protostars may be analogous to our proto-Sun and…

2019 Monthly Notices of the Royal Astronomical Society
Rosetta 119
The origin of galactic metal-rich stellar halo components with highly eccentric orbits
DOI: 10.1093/mnras/stz159 Bibcode: 2019MNRAS.484.4471F

Springel, Volker; Grand, Robert J. J.; Gómez, Facundo A. +6 more

Using the astrometry from the ESA's Gaia mission, previous works have shown that the Milky Way stellar halo is dominated by metal-rich stars on highly eccentric orbits. To shed light on the nature of this prominent halo component, we have analysed 28 Galaxy analogues in the Auriga suite of cosmological hydrodynamics zoom-in simulations. Some three…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 118
Piercing the Milky Way: an all-sky view of the Orphan Stream
DOI: 10.1093/mnras/stz457 Bibcode: 2019MNRAS.485.4726K

Li, T. S.; Evans, N. W.; Belokurov, V. +14 more

We use astrometry, broad-band photometry, and variability information from the Data Release 2 of ESA's Gaia mission (GDR2) to identify members of the Orphan Stream (OS) across the whole sky. The stream is traced above and below the celestial equator and in both Galactic hemispheres, thus increasing its visible length to ∼210° equivalent to ∼150 kp…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 114
The Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters - XIX. A chemical tagging of the multiple stellar populations over the chromosome maps
DOI: 10.1093/mnras/stz1415 Bibcode: 2019MNRAS.487.3815M

Anderson, J.; Milone, A. P.; Cordoni, G. +8 more

The Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters (GCs) has investigated GCs and their stellar populations. In previous papers of this series we have introduced a pseudo two-colour diagram, or `chromosome map' (ChM) that maximizes the separation between the multiple populations. We have identified two main classes of GCs: T…

2019 Monthly Notices of the Royal Astronomical Society
Gaia eHST 114
Homogeneous photometry - VII. Globular clusters in the Gaia era
DOI: 10.1093/mnras/stz585 Bibcode: 2019MNRAS.485.3042S

Pancino, E.; Sanna, N.; Stetson, P. B. +2 more

We present wide-field, ground-based Johnson-Cousins UBVRI photometry for 48 Galactic globular clusters based on about 90 000 public and proprietary images. The photometry is calibrated with the latest transformations obtained in the framework of our secondary standard project, with typical internal and external uncertainties of order a few millima…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 114