Search Publications

Forming Super Star Clusters in the Central Starburst of NGC 253
DOI: 10.3847/1538-4357/aaecd1 Bibcode: 2018ApJ...869..126L

Meier, David S.; Ott, Jürgen; Bolatto, Alberto D. +12 more

NGC 253 hosts the nearest nuclear starburst. Previous observations show a region rich in molecular gas, with dense clouds associated with recent star formation. We used the Atacama Large Submillimeter/Millimeter Array (ALMA) to image the 350 GHz dust continuum and molecular line emission from this region at 2 pc resolution. Our observations reveal…

2018 The Astrophysical Journal
eHST 95
The Diversity of Kilonova Emission in Short Gamma-Ray Bursts
DOI: 10.3847/1538-4357/aac206 Bibcode: 2018ApJ...860...62G

Covino, S.; Lyman, J. D.; Fruchter, A. S. +10 more

The historic first joint detection of both gravitational-wave and electromagnetic emission from a binary neutron star merger cemented the association between short gamma-ray bursts (SGRBs) and compact object mergers, as well as providing a well-sampled multi-wavelength light curve of a radioactive kilonova (KN) for the first time. Here, we compare…

2018 The Astrophysical Journal
eHST 94
Fast and Slow Paths to Quiescence: Ages and Sizes of 400 Quiescent Galaxies from the LEGA-C Survey
DOI: 10.3847/1538-4357/aae822 Bibcode: 2018ApJ...868...37W

Bell, Eric F.; Franx, Marijn; Muzzin, Adam +11 more

We analyze the stellar age indicators (D n 4000 and EW(Hδ)) and sizes of 467 quiescent galaxies with M * ≥ 1010 M at z ∼ 0.7 drawn from DR2 of the LEGA-C survey. Interpreting index variations in terms of equivalent single stellar population age, we find that the median stellar population is younger for…

2018 The Astrophysical Journal
eHST 92
On the Gas Content and Efficiency of AGN Feedback in Low-redshift Quasars
DOI: 10.3847/1538-4357/aaa9be Bibcode: 2018ApJ...854..158S

Ho, Luis C.; Shangguan, Jinyi; Xie, Yanxia

The interstellar medium is crucial to understanding the physics of active galaxies and the coevolution between supermassive black holes and their host galaxies. However, direct gas measurements are limited by sensitivity and other uncertainties. Dust provides an efficient indirect probe of the total gas. We apply this technique to a large sample o…

2018 The Astrophysical Journal
Herschel 92
Homogeneous Analysis of the Dust Morphology of Transition Disks Observed with ALMA: Investigating Dust Trapping and the Origin of the Cavities
DOI: 10.3847/1538-4357/aabf94 Bibcode: 2018ApJ...859...32P

van der Plas, G.; Pascucci, I.; Garufi, A. +11 more

We analyze the dust morphology of 29 transition disks (TDs) observed with Atacama Large (sub-)Millimeter Array (ALMA) at (sub-)millimeter emission. We perform the analysis in the visibility plane to characterize the total flux, cavity size, and shape of the ring-like structure. First, we found that the M dust-M relation is …

2018 The Astrophysical Journal
Gaia 92
Non-negative Matrix Factorization: Robust Extraction of Extended Structures
DOI: 10.3847/1538-4357/aaa1f2 Bibcode: 2018ApJ...852..104R

Duchêne, Gaspard; Pueyo, Laurent; Debes, John +2 more

We apply the vectorized non-negative matrix factorization (NMF) method to the post-processing of the direct imaging data of exoplanetary systems such as circumstellar disks. NMF is an iterative approach, which first creates a nonorthogonal and non-negative basis of components using the given reference images and then models a target with the compo…

2018 The Astrophysical Journal
eHST 92
The CO Luminosity Density at High-z (COLDz) Survey: A Sensitive, Large-area Blind Search for Low-J CO Emission from Cold Gas in the Early Universe with the Karl G. Jansky Very Large Array
DOI: 10.3847/1538-4357/aacb79 Bibcode: 2018ApJ...864...49P

Dickinson, Mark; Smail, Ian; Daddi, Emanuele +16 more

We describe the CO Luminosity Density at High-z (COLDz) survey, the first spectral line deep field targeting CO(1-0) emission from galaxies at z = 1.95-2.85 and CO(2-1) at z = 4.91-6.70. The main goal of COLDz is to constrain the cosmic density of molecular gas at the peak epoch of cosmic star formation. By targeting both a wide (∼51 arcmin2<…

2018 The Astrophysical Journal
eHST 91
Production of Cool Gas in Thermally Driven Outflows
DOI: 10.3847/1538-4357/aacce1 Bibcode: 2018ApJ...862...56S

Robertson, Brant E.; Thompson, Todd A.; Schneider, Evan E.

Galactic outflows commonly contain multiphase gas, and its physical origin requires explanation. Using the Cholla Galactic OutfLow Simulations suite of high-resolution isolated galaxy models, we demonstrate the viability of rapid radiative cooling as a source of fast-moving (v ∼ 1000 km s-1), cool (104 K) gas observed in abso…

2018 The Astrophysical Journal
eHST 91
Hubble Space Telescope Observations of Extended [O III]λ 5007 Emission in Nearby QSO2s: New Constraints on AGN Host Galaxy Interaction
DOI: 10.3847/1538-4357/aab03e Bibcode: 2018ApJ...856..102F

Turner, T. J.; Kraemer, S. B.; Crenshaw, D. M. +15 more

We present a Hubble Space Telescope survey of extended [O III] λ5007 emission for a sample of 12 nearby (z < 0.12), luminous Type 2 quasars (QSO2s), which we use to measure the extent and kinematics of their AGN-ionized gas. We find that the size of the observed [O III] regions scale with luminosity in comparison to nearby, less luminous Seyfer…

2018 The Astrophysical Journal
eHST 90
Successive X-class Flares and Coronal Mass Ejections Driven by Shearing Motion and Sunspot Rotation in Active Region NOAA 12673
DOI: 10.3847/1538-4357/aab153 Bibcode: 2018ApJ...856...79Y

Feng, X. S.; Yan, X. L.; Xue, Z. K. +5 more

We present a clear case study on the occurrence of two successive X-class flares, including a decade-class flare (X9.3) and two coronal mass ejections (CMEs) triggered by shearing motion and sunspot rotation in active region NOAA 12673 on 2017 September 6. A shearing motion between the main sunspots with opposite polarities began on September 5 an…

2018 The Astrophysical Journal
SOHO 90