Search Publications

A Fully Kinetic Perspective of Electron Acceleration around a Weakly Outgassing Comet
DOI: 10.3847/2041-8213/ab6662 Bibcode: 2020ApJ...889L..33D

Henri, Pierre; Lapenta, Giovanni; Divin, Andrey +4 more

The cometary mission Rosetta has shown the presence of higher-than-expected suprathermal electron fluxes. In this study, using 3D fully kinetic electromagnetic simulations of the interaction of the solar wind with a comet, we constrain the kinetic mechanism that is responsible for the bulk electron energization that creates the suprathermal distri…

2020 The Astrophysical Journal
Rosetta 15
The Origin of a Distributed Stellar Population in the Star-forming Region W4
DOI: 10.3847/1538-4357/aba0a3 Bibcode: 2020ApJ...899..121L

Lim, Beomdu; Lee, Jeong-Eun; Yun, Hyeong-Sik +5 more

Stellar kinematics provides the key to understanding the formation process and dynamical evolution of stellar systems. Here, we present a kinematic study of the massive star-forming region (SFR) W4 in the Cassiopeia OB6 association using the Gaia Data Release 2 and high-resolution optical spectra. This SFR is composed of a core cluster (IC 1805) a…

2020 The Astrophysical Journal
Gaia 15
2003-2019 Monitoring of the Crab Emission through INTEGRAL SPI, or Vice Versa
DOI: 10.3847/1538-4357/aba8a4 Bibcode: 2020ApJ...899..131J

Jourdain, E.; Roques, J. P.

The Crab Nebula is used by many instruments as a calibration source, in particular at high energy, where it is one of the brightest celestial objects. The spectrometer INTEGRAL SPI (20 keV-8 MeV), in operation since 2002 October, offers a large data set dedicated to this source, with regular campaigns planned twice per year. We have analyzed the a…

2020 The Astrophysical Journal
INTEGRAL 15
The Not So Simple Stellar System ω Cen. II. Evidence in Support of a Merging Scenario
DOI: 10.3847/1538-4357/ab77c0 Bibcode: 2020ApJ...891..167C

Rest, Armin; Mastrobuono-Battisti, Alessandra; Zenteno, Alfredo +7 more

We present multiband photometry covering ∼5° × 5° across ω Cen collected with the Dark Energy Camera on the 4 m Blanco telescope, combined with Hubble Space Telescope and Wide Field Imager data for the central regions. The unprecedented photometric accuracy and field coverage allows us to confirm the different spatial distribution of blue and red …

2020 The Astrophysical Journal
Gaia eHST 15
When Does the Onset of Multiple Stellar Populations in Star Clusters Occur? III. No Evidence of Significant Chemical Variations in Main-sequence Stars of NGC 419
DOI: 10.3847/1538-4357/ab7b64 Bibcode: 2020ApJ...893...17L

Milone, Antonino P.; Li, Chengyuan; Ji, Xin +3 more

Recent studies have revealed that the onset age for the presence of multiple stellar populations (MPs) in star clusters seems to correspond to the disappearance of the extended main-sequence turnoff in young clusters, a pattern associated with stellar rotations. A speculative suggestion is that MPs might be caused by the magnetic brake, a stellar …

2020 The Astrophysical Journal
eHST 15
Rotation of Solar Analogs Crossmatching Kepler and Gaia DR2
DOI: 10.3847/1538-4357/ab9c16 Bibcode: 2020ApJ...898..173D

Barnes, S. A.; Castro, M.; da Costa, J. S. +10 more

A major obstacle to interpreting the rotation period distribution for main-sequence stars from Kepler mission data has been the lack of a precise evolutionary status for these objects. We address this by investigating the evolutionary status based on Gaia Data Release 2 parallaxes and photometry for more than 30,000 Kepler stars with rotation peri…

2020 The Astrophysical Journal
Gaia 15
A Tale of Two Transition Disks: ALMA Long-baseline Observations of ISO-Oph 2 Reveal Two Closely Packed Nonaxisymmetric Rings and a ∼2 au Cavity
DOI: 10.3847/2041-8213/abbcce Bibcode: 2020ApJ...902L..33G

Flock, Mario; Herczeg, Gregory J.; Pinilla, Paola +12 more

ISO-Oph 2 is a wide-separation (240 au) binary system where the primary star harbors a massive (Mdust ∼ 40 M) ring-like disk with a dust cavity ∼50 au in radius and the secondary hosts a much lighter (Mdust ∼ 0.8 M) disk. As part of the high-resolution follow-up of the "Ophiuchus Disk Survey Employing …

2020 The Astrophysical Journal
Gaia 15
Molecular Gas Outflow in the Starburst Galaxy NGC 1482
DOI: 10.3847/1538-4357/abb134 Bibcode: 2020ApJ...901..151S

Salak, Dragan; Nakai, Naomasa; Miyamoto, Yusuke +1 more

Galactic winds are essential to the regulation of star formation in galaxies. To study the distribution and dynamics of molecular gas in wind, we imaged the nearby starburst galaxy NGC 1482 in CO (J = 1 → 0) at a resolution of 1″ (≈100 pc) using the Atacama Large Millimeter/submillimeter Array. Molecular gas is detected in a nearly edge-on disk wi…

2020 The Astrophysical Journal
eHST 15
Characterizing the Circumgalactic Medium of the Lowest-mass Galaxies: A Case Study of IC 1613
DOI: 10.3847/1538-4357/abc875 Bibcode: 2020ApJ...905..133Z

Putman, Mary E.; Kirby, Evan N.; Werk, Jessica K. +3 more

Using 10 sight lines observed with the Hubble Space Telescope/Cosmic Origins Spectrograph, we study the circumgalactic medium (CGM) and outflows of IC 1613, which is a low-mass (M* ∼ 108 M), dwarf irregular galaxy on the outskirts of the Local Group. Among the sight lines, four are pointed toward UV-bright stars i…

2020 The Astrophysical Journal
eHST 15
Confirmation of Enhanced Long-wavelength Dust Emission in OMC 2/3
DOI: 10.3847/1538-4357/ab734a Bibcode: 2020ApJ...893...13M

Friesen, Rachel; Sadavoy, Sarah; Mroczkowski, Tony +8 more

Previous continuum observations from the MUSTANG camera on the Green Bank Telescope (GBT) of the nearby star-forming filament OMC 2/3 found elevated emission at 3.3 mm relative to shorter-wavelength data. As a consequence, the inferred dust emissivity index obtained from modified blackbody dust spectra was considerably lower than what is typically…

2020 The Astrophysical Journal
Herschel 15