Search Publications

The ALMA Spectroscopic Survey in the HUDF: Nature and Physical Properties of Gas-mass Selected Galaxies Using MUSE Spectroscopy
DOI: 10.3847/1538-4357/ab3102 Bibcode: 2019ApJ...882..140B

Carilli, Chris; Somerville, Rachel S.; Bacon, Roland +31 more

We discuss the nature and physical properties of gas-mass selected galaxies in the ALMA spectroscopic survey (ASPECS) of the Hubble Ultra Deep Field (HUDF). We capitalize on the deep optical integral-field spectroscopy from the Multi Unit Spectroscopic Explorer (MUSE) HUDF Survey and multiwavelength data to uniquely associate all 16 line emitters,…

2019 The Astrophysical Journal
eHST 58
Validation of the Alfvén Wave Solar Atmosphere Model (AWSoM) with Observations from the Low Corona to 1 au
DOI: 10.3847/1538-4357/ab4f5e Bibcode: 2019ApJ...887...83S

van der Holst, Bart; Lamy, Philippe; Vásquez, Alberto M. +9 more

We perform a validation study of the latest version of the Alfvén Wave Solar atmosphere Model (AWSoM) within the Space Weather Modeling Framework. To do so, we compare the simulation results of the model with a comprehensive suite of observations for Carrington rotations representative of the solar minimum conditions extending from the solar coron…

2019 The Astrophysical Journal
SOHO Ulysses 58
Emergence of the Gaia phase space spirals from bending waves
DOI: 10.1093/mnras/sty3508 Bibcode: 2019MNRAS.484.1050D

Widrow, Lawrence M.; Darling, Keir

We discuss the physical mechanism by which pure vertical bending waves in a stellar disc evolve to form phase space spirals similar to those discovered by Antoja et al. in Gaia Data Release 2. These spirals are found by projecting Solar Neighbourhood stars on to the z-vz plane. Faint spirals appear in the number density of stars project…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 58
On the nature and physical conditions of the luminous Ly α emitter CR7 and its rest-frame UV components
DOI: 10.1093/mnras/sty2779 Bibcode: 2019MNRAS.482.2422S

Ferrara, Andrea; Schaerer, Daniel; Sobral, David +6 more

We present new Hubble Space Telescope (HST)/WFC3 observations and re-analyse VLT data to unveil the continuum, variability, and rest-frame ultraviolet (UV) lines of the multiple UV clumps of the most luminous Ly α emitter at z = 6.6, CR7 (COSMOS Redshift 7). Our re-reduced, flux-calibrated X-SHOOTER spectra of CR7 reveal an He II emission line in …

2019 Monthly Notices of the Royal Astronomical Society
eHST 58
A Catalog of OB Stars from LAMOST Spectroscopic Survey
DOI: 10.3847/1538-4365/ab0a0d Bibcode: 2019ApJS..241...32L

Zhao, Gang; Huang, Yang; Liu, Chao +3 more

We present 22,901 OB spectra of 16,032 stars identified from the Large Sky Area Multi-Object Fiber Spectroscopic Telescope data release 5 data set. A larger sample of OB candidates are first selected from the distributions in the spectral line indices’ space. Then, all 22,901 OB spectra are identified by manual inspection. Based on a subsample val…

2019 The Astrophysical Journal Supplement Series
Gaia 58
Gaia kinematics reveal a complex lopsided and twisted Galactic disc warp
DOI: 10.1051/0004-6361/201834908 Bibcode: 2019A&A...627A.150R

Castro-Ginard, A.; Figueras, F.; Romero-Gómez, M. +2 more

Context. There are few warp kinematic models of the Galaxy able to characterise both structure and kinematics, since these require high accuracy at large distances. These models are necessary to shed light on the lopsidedness of the warp and the twisting of the line-of-nodes of the stellar warp already seen in gas and dust.
Aims: We use the v…

2019 Astronomy and Astrophysics
Gaia 58
Global 3D Hydrodynamic Modeling of In-transit Lyα Absorption of GJ 436b
DOI: 10.3847/1538-4357/ab46a4 Bibcode: 2019ApJ...885...67K

Lammer, H.; Khodachenko, M. L.; Shaikhislamov, I. F. +5 more

Using a global 3D, fully self-consistent, multifluid hydrodynamic model, we simulate the escaping upper atmosphere of the warm Neptune GJ 436b, driven by the stellar X-ray and ultraviolet (XUV) radiation impact and gravitational forces and interacting with the stellar wind. Under the typical parameters of XUV flux and stellar wind plasma expected …

2019 The Astrophysical Journal
eHST 58
Morphologies of ∼190,000 Galaxies at z = 0-10 Revealed with HST Legacy Data. III. Continuum Profile and Size Evolution of Lyα Emitters
DOI: 10.3847/1538-4357/aaf64b Bibcode: 2019ApJ...871..164S

Ouchi, Masami; Harikane, Yuichi; Shibuya, Takatoshi +1 more

We present the redshift evolution of the radial surface brightness profile of the rest-frame UV and optical stellar continua for 9119 Lyα emitters (LAEs) at z ≃ 0-8 and 0-2, respectively. Using Hubble Space Telescope data and the LAE catalogs taken from the literature, we derive the structural quantities of the 9119 LAEs, and of ≃180,000 of photo-…

2019 The Astrophysical Journal
eHST 58
Nuclear molecular outflow in the Seyfert galaxy NGC 3227
DOI: 10.1051/0004-6361/201935431 Bibcode: 2019A&A...628A..65A

Rigopoulou, D.; Hunt, L. K.; Vestergaard, M. +24 more

ALMA observations have revealed nuclear dusty molecular disks or tori with characteristic sizes 15-40 pc in the few Seyferts and low -luminosity AGN that have been studied so far. These structures are generally decoupled both morphologically and kinematically from the host galaxy disk. We present ALMA observations of the CO(2-1) and CO(3-2) molecu…

2019 Astronomy and Astrophysics
eHST 58
Boötes. IV. A new Milky Way satellite discovered in the Subaru Hyper Suprime-Cam Survey and implications for the missing satellite problem
DOI: 10.1093/pasj/psz076 Bibcode: 2019PASJ...71...94H

Strauss, Michael A.; Wang, Shiang-Yu; Ishigaki, Miho N. +13 more

We report on the discovery of a new Milky Way (MW) satellite in Boötes based on data from the ongoing Hyper Suprime-Cam (HSC) Subaru Strategic Program (SSP). This satellite, named Boötes IV, is the third ultra-faint dwarf that we have discovered in the HSC-SSP. We have identified a statistically significant (32.3σ) overdensity of stars with charac…

2019 Publications of the Astronomical Society of Japan
eHST 58