Search Publications

Hubble Ultraviolet Spectroscopy of Jupiter Trojans
DOI: 10.3847/1538-3881/ab0e00 Bibcode: 2019AJ....157..161W

Ehlmann, Bethany L.; Brown, Michael E.; Mahjoub, Ahmed +2 more

We present the first ultraviolet spectra of Jupiter Trojans. These observations were carried out using the Space Telescope Imaging Spectrograph on the Hubble Space Telescope and cover the wavelength range 200-550 nm at low resolution. The targets include objects from both of the Trojan color subpopulations (less-red and red). We do not observe any…

2019 The Astronomical Journal
eHST 17
Variability of young stellar objects in the star-forming region Pelican Nebula
DOI: 10.1051/0004-6361/201935418 Bibcode: 2019A&A...627A.135B

Chen, W. P.; Herczeg, G. J.; Bhardwaj, A. +2 more

Context. Pre-main-sequence variability characteristics can be used to probe the physical processes leading to the formation and initial evolution of both stars and planets.
Aims: The photometric variability of pre-main-sequence stars is studied at optical wavelengths to explore star-disk interactions, accretion, spots, and other physical mech…

2019 Astronomy and Astrophysics
Gaia 17
Antlia 2’s Role in Driving the Ripples in the Outer Gas Disk of the Galaxy
DOI: 10.3847/1538-4357/ab4659 Bibcode: 2019ApJ...886...67C

Hernquist, Lars; Price-Whelan, Adrian M.; Chang, Philip +3 more

We employ the earlier published proper motions of the newly discovered Antlia 2 dwarf galaxy derived from Gaia data to calculate its orbital distribution in the cosmologically recent past. Using these observationally motivated orbits, we calculate the effect of the Antlia 2 dwarf galaxy on the outer H I disk of the Milky Way, using both test parti…

2019 The Astrophysical Journal
Gaia 17
Hyperluminous starburst gives up its secrets
DOI: 10.1093/mnras/stz2180 Bibcode: 2019MNRAS.489..427I

Ivison, R. J.; Page, M. J.; Mainieri, V. +4 more

HATLAS J084933.4 + 021443 was identified as a dusty starburst via its rest-frame far-infrared (far-IR) emission. Multifrequency imaging and spectroscopy revealed a cluster of four dusty galaxies at z = 2.41, covering 80 kpc. Here, we use Atacama Large Millimetre Array to confirm a more distant, fifth protocluster member, and present X-ray and rest…

2019 Monthly Notices of the Royal Astronomical Society
XMM-Newton 17
Learning mid-IR emission spectra of polycyclic aromatic hydrocarbon populations from observations
DOI: 10.1051/0004-6361/201935085 Bibcode: 2019A&A...632A..84F

Joblin, C.; Berné, O.; Foschino, S.

Context. The James Webb Space Telescope (JWST) will deliver an unprecedented quantity of high-quality spectral data over the 0.6-28 µm range. It will combine sensitivity, spectral resolution, and spatial resolution. Specific tools are required to provide efficient scientific analysis of such large data sets.
Aims: Our aim is to illustra…

2019 Astronomy and Astrophysics
ISO 17
SPIRE Spectroscopy of Early-type Galaxies
DOI: 10.3847/1538-4357/ab0d23 Bibcode: 2019ApJ...875....3L

Young, Lisa M.; Lapham, Ryen Carl

We present Spectral and Photometric Imaging Receiver (SPIRE) spectroscopy for nine early-type galaxies (ETGs) representing the most CO-rich and far-infrared (FIR) bright galaxies of the volume-limited Atlas3D sample. Our data include detections of mid- to high-J CO transitions (J = 4-3 to J = 13-12) and the [C I] (1-0) and (2-1) emission lines. CO…

2019 The Astrophysical Journal
Herschel 17
The z = 0.54 LoBAL Quasar SDSS J085053.12+445122.5. II. The Nature of Partial Covering in the Broad-absorption-line Outflow
DOI: 10.3847/1538-4357/ab212a Bibcode: 2019ApJ...879...27L

Gallagher, Sarah C.; Terndrup, Donald M.; Leighly, Karen M. +5 more

It has been known for 20 years that the absorbing gas in broad-absorption-line quasars does not completely cover the continuum emission region, and that partial covering must be accounted for to accurately measure the column density of the outflowing gas. However, the nature of partial covering itself is not understood. Extrapolation of the SimBAL…

2019 The Astrophysical Journal
eHST 17
HADES RV Programme with HARPS-N at TNG. X. The non-saturated regime of the stellar activity-rotation relationship for M dwarfs
DOI: 10.1051/0004-6361/201834386 Bibcode: 2019A&A...624A..27G

Rebolo, R.; Ribas, I.; Scandariato, G. +22 more


Aims: We extend the relationship between X-ray luminosity (Lx) and rotation period (Prot) found for main-sequence FGK stars, and test whether it also holds for early M dwarfs, especially in the non-saturated regime (Lx ∝ Prot-2) which corresponds to slow rotators.
Methods: We use the…

2019 Astronomy and Astrophysics
XMM-Newton 17
The Nearby, Young, χ 1 Fornacis Cluster: Membership, Age, and an Extraordinary Ensemble of Dusty Debris Disks
DOI: 10.3847/1538-4357/ab45ea Bibcode: 2019ApJ...887...87Z

Zuckerman, B.; Kastner, Joel; Klein, Beth

Only four star clusters are known within ∼100 pc of Earth. Of these, the χ 1 For cluster has barely been studied. We use the Gaia DR2 catalog and other published data to establish the cluster membership, structure, and age. The age of and distance to the cluster are ∼40 Myr and 104 pc, respectively. A remarkable, unprecedented aspect of…

2019 The Astrophysical Journal
Gaia XMM-Newton 17
A Very Large Array Survey of Luminous Extranuclear Star-forming Regions in Luminous Infrared Galaxies in GOALS
DOI: 10.3847/1538-4357/ab2872 Bibcode: 2019ApJ...881...70L

Surace, J. A.; Murphy, E. J.; Momjian, E. +13 more

We present the first results of a high-resolution Karl G. Jansky Very Large Array imaging survey of luminous and ultra-luminous infrared galaxies (U/LIRGs) in the Great Observatories All-sky LIRG Survey. From the full sample of 68 galaxies, we have selected 25 luminous infrared galaxies (LIRGs) that show resolved extended emission at sufficient se…

2019 The Astrophysical Journal
eHST 17