Search Publications

The Star Formation History in the Solar Neighborhood as Told by Massive White Dwarfs
DOI: 10.3847/2041-8213/ab238e Bibcode: 2019ApJ...878L..11I

Isern, Jordi

White dwarfs (WDs) are the remnants of low- and intermediate-mass stars. Because of electron degeneracy, their evolution is just a simple gravothermal process of cooling. Recently, thanks to Gaia data, it has been possible to construct the luminosity function of massive (0.9≤slant M/{M}≤slant 1.1) WDs in the solar neighborhood (d< …

2019 The Astrophysical Journal
Gaia 45
Evolved massive stars at low-metallicity. I. A source catalog for the Small Magellanic Cloud
DOI: 10.1051/0004-6361/201935916 Bibcode: 2019A&A...629A..91Y

Yang, Ming; Bonanos, Alceste Z.; Jiang, Bi-Wei +9 more

We present a clean, magnitude-limited (IRAC1 or WISE1 ≤ 15.0 mag) multiwavelength source catalog for the Small Magellanic Cloud (SMC) with 45 466 targets in total, with the purpose of building an anchor for future studies, especially for the massive star populations at low-metallicity. The catalog contains data in 50 different bands including 21 o…

2019 Astronomy and Astrophysics
AKARI Gaia Herschel 45
Distances to molecular clouds at high galactic latitudes based on Gaia DR2
DOI: 10.1051/0004-6361/201834337 Bibcode: 2019A&A...624A...6Y

Macquart, Jean-Pierre; Xu, Ye; Yan, Qing-Zeng +4 more

We report the distances of molecular clouds at high Galactic latitudes (|b| > 10°) derived from parallax and G-band extinction (AG) measurements in the second Gaia data release, Gaia DR2. Aided by Bayesian analyses, we determined distances by identifying the breakpoint in the extinction AG toward molecular clouds and using…

2019 Astronomy and Astrophysics
Gaia 45
Probing fragmentation and velocity sub-structure in the massive NGC 6334 filament with ALMA
DOI: 10.1051/0004-6361/201935689 Bibcode: 2019A&A...632A..83S

André, Ph.; Arzoumanian, D.; Shimajiri, Y. +3 more

Context. Herschel imaging surveys of galactic interstellar clouds support a paradigm for low-mass star formation in which dense molecular filaments play a crucial role. The detailed fragmentation properties of star-forming filaments remain poorly understood, however, and the validity of the filament paradigm in the intermediate- to high-mass regim…

2019 Astronomy and Astrophysics
Herschel 44
The Fraction of Active Galactic Nuclei in the USS 1558-003 Protocluster at z = 2.53
DOI: 10.3847/1538-4357/ab0746 Bibcode: 2019ApJ...874...54M

Miller, Eric D.; Koyama, Yusei; Kodama, Tadayuki +8 more

The incidence of active galactic nuclei (AGNs) within the local environment is a potentially valuable probe of the mechanisms that trigger and provide fuel for accretion onto supermassive black holes. While the correlation between AGN fraction and environment has been well-studied in the local universe, AGN fractions have been measured for relativ…

2019 The Astrophysical Journal
eHST 44
The metal-rich atmosphere of the exo-Neptune HAT-P-26b
DOI: 10.1093/mnras/stz789 Bibcode: 2019MNRAS.486.1292M

Madhusudhan, Nikku; MacDonald, Ryan J.

Transmission spectroscopy is enabling precise measurements of atmospheric H2O abundances for numerous giant exoplanets. For hot Jupiters, relating H2O abundances to metallicities provides a powerful probe of their formation conditions. However, metallicity measurements for Neptune-mass exoplanets are only now becoming viable.…

2019 Monthly Notices of the Royal Astronomical Society
eHST 44
METAL: The Metal Evolution, Transport, and Abundance in the Large Magellanic Cloud Hubble Program. I. Overview and Initial Results
DOI: 10.3847/1538-4357/aaf8bb Bibcode: 2019ApJ...871..151R

Jenkins, Edward B.; Yanchulova Merica-Jones, Petia; Meixner, Margaret +8 more

Metal Evolution, Transport, and Abundance in the LMC (METAL) is a large Cycle 24 program on the Hubble Space Telescope aimed at measuring dust extinction properties and interstellar depletions in the Large Magellanic Cloud (LMC) at half-solar metallicity. The 101-orbit program is composed of Cosmic Origins Spectrograph and Space Telescope Imaging …

2019 The Astrophysical Journal
Herschel eHST 44
Warm FIRE: simulating galaxy formation with resonant sterile neutrino dark matter
DOI: 10.1093/mnras/sty3300 Bibcode: 2019MNRAS.483.4086B

Faucher-Giguère, Claude-André; Hopkins, Philip F.; Wetzel, Andrew +8 more

We study the impact of a warm dark matter (WDM) cosmology on dwarf galaxy formation through a suite of cosmological hydrodynamical zoom-in simulations of M_halo ≈ 10^{10} M_{⊙} dark matter haloes as part of the Feedback in Realistic Environments (FIRE) project. A main focus of this paper is to evaluate the combined effects of dark matter physics a…

2019 Monthly Notices of the Royal Astronomical Society
eHST 44
Photochemical Hazes in Sub-Neptunian Atmospheres with a Focus on GJ 1214b
DOI: 10.3847/1538-4357/ab204e Bibcode: 2019ApJ...878..118L

Showman, Adam P.; García Muñoz, Antonio; Steinrueck, Maria E. +2 more

We study the properties of photochemical hazes in super-Earth/mini-Neptune atmospheres with particular focus on GJ 1214b. We evaluate photochemical haze properties at different metallicities between solar and 10,000× solar. Within the four-order-of-magnitude change in metallicity, we find that the haze precursor mass fluxes change only by a factor…

2019 The Astrophysical Journal
eHST 44
The Sporadic Activity of (6478) Gault: A YORP-driven Event?
DOI: 10.3847/2041-8213/ab0f40 Bibcode: 2019ApJ...874L..20K

Wainscoat, Richard J.; Tonry, John; Ebeling, Harald +15 more

On 2019 January 5 a streamer associated with the 4-10 km main belt asteroid (6478) Gault was detected by the ATLAS sky survey, a rare discovery of activity around a main belt asteroid. Archival data from ATLAS and Pan-STARRS1 show the trail in early 2018 December, but not between 2010 and 2018 January. The feature has significantly changed over on…

2019 The Astrophysical Journal
eHST 44