Search Publications

CANDELS Meets GSWLC: Evolution of the Relationship between Morphology and Star Formation Since z = 2
DOI: 10.3847/1538-4357/abb5af Bibcode: 2020ApJ...902...77O

Faber, S. M.; Tacchella, Sandro; Salim, Samir +7 more

Galaxy morphology and its evolution over the cosmic epoch hold important clues for understanding the regulation of star formation (SF). However, studying the relationship between morphology and SF has been hindered by the availability of consistent data at different redshifts. Our sample, combining CANDELS (0.8 < z < 2.5) and the GALEX-SDSS-…

2020 The Astrophysical Journal
eHST 17
Can Subphotospheric Magnetic Reconnection Change the Elemental Composition in the Solar Corona?
DOI: 10.3847/1538-4357/ab7dcb Bibcode: 2020ApJ...894...35B

Long, David M.; Brooks, David H.; Baker, Deborah +6 more

Within the coronae of stars, abundances of those elements with low first ionization potential (FIP) often differ from their photospheric values. The coronae of the Sun and solar-type stars mostly show enhancements of low-FIP elements (the FIP effect) while more active stars such as M dwarfs have coronae generally characterized by the inverse-FIP e…

2020 The Astrophysical Journal
Hinode 17
Electron Temperature Anisotropy and Electron Beam Constraints from Electron Kinetic Instabilities in the Solar Wind
DOI: 10.3847/1538-4357/abb3ca Bibcode: 2020ApJ...902...59S

Xie, Huasheng; Wu, Dejin; Sun, Heyu +2 more

Electron temperature anisotropies and electron beams are nonthermal features of the observed nonequilibrium electron velocity distributions in the solar wind. In collision-poor plasmas these nonequilibrium distributions are expected to be regulated by kinetic instabilities through wave-particle interactions. This study considers electron instabili…

2020 The Astrophysical Journal
Cluster 17
Helium Line Emissivities in the Solar Corona
DOI: 10.3847/1538-4357/ab9d84 Bibcode: 2020ApJ...898...72D

Andretta, V.; Del Zanna, G.; Storey, P. J. +1 more

We present new collisional-radiative models (CRMs) for helium in the quiescent solar corona and predict the emissivities of the He and He+ lines to be observed by DKIST, Solar Orbiter, and Proba-3. We discuss in detail the rates we selected for these models, highlighting several shortcomings we have found in previous work. As no previou…

2020 The Astrophysical Journal
SOHO 17
On the Diversity of Jet Production Efficiency in Swift/BAT AGNs
DOI: 10.3847/1538-4357/aba75f Bibcode: 2020ApJ...900..125R

Sikora, Marek; Gupta, Maitrayee; Rusinek, Katarzyna +1 more

We address the very large diversity of jet production efficiency in active galactic nuclei (AGNs) by using data on low-redshift AGNs selected from the Swift/BAT catalog and having black hole (BH) masses larger than 108.5 M. Most of these AGNs accrete at intermediate rates and have bolometric luminosities dominated by mid-IR …

2020 The Astrophysical Journal
eHST 17
The Extreme Red Excess in Blazar Ultraviolet Broad Emission Lines
DOI: 10.3847/1538-4357/abb950 Bibcode: 2020ApJ...903...44P

Berton, Marco; Punsly, Brian; Marziani, Paola +1 more

We present a study of quasars with very redward asymmetric (RA) ultraviolet (UV) broad emission lines (BELs). An excess of redshifted emission has been previously shown to occur in the BELs of radio-loud quasars and is most extreme in certain blazars. Paradoxically, blazars are objects that are characterized by a highly relativistic blueshifted ou…

2020 The Astrophysical Journal
INTEGRAL eHST 17
ALMA Observations of Young Eruptive Stars: Continuum Disk Sizes and Molecular Outflows
DOI: 10.3847/1538-4357/aba3c4 Bibcode: 2020ApJ...900....7H

Hales, Antonio S.; Pérez, Sebastián; Gonzalez-Ruilova, Camilo +7 more

We present Atacama Large Millimeter/submillimeter Array (ALMA) 1.3 mm observations of four young, eruptive star-disk systems at 0"4 resolution: two FUors (V582 Aur and V900 Mon), one EXor (UZ Tau E), and one source with an ambiguous FU/EXor classification (GM Cha). The disks around GM Cha, V900 Mon, and UZ Tau E are resolved. These observations in…

2020 The Astrophysical Journal
Gaia 17
On the Ratios of Si IV Lines (λ1394/λ1403) in an Emerging Flux Region
DOI: 10.3847/1538-4357/ab8558 Bibcode: 2020ApJ...894..128T

Isobe, Hiroaki; Tripathi, Durgesh; Nived, V. N. +1 more

The resonance lines of Si IV formed at λ1394 and 1403 Å are the most critical for the diagnostics of the solar transition region in the observations of the Interface Region Imaging Spectrograph (IRIS). Studying the intensity ratios of these lines (1394 Å/1403 Å), which under optically thin conditions is predicted to be two, helps us to diagnose th…

2020 The Astrophysical Journal
IRIS 17
The Extreme CNO-enhanced Composition of the Primitive Iron-poor Dwarf Star J0815+4729
DOI: 10.3847/2041-8213/ab62ae Bibcode: 2020ApJ...889L..13G

Burgasser, Adam J.; Aguado, David S.; Allende Prieto, Carlos +2 more

We present an analysis of high-resolution Keck/HIRES spectroscopic observations of J0815+4729, an extremely carbon-enhanced, iron-poor dwarf star. These high-quality data allow us to derive a metallicity of [Fe/H] = -5.49 ± 0.14 from the three strongest Fe I lines and to measure a high [Ca/Fe] = 0.75 ± 0.14. The large carbon abundance of A(C) = 7.…

2020 The Astrophysical Journal
Gaia 17
A Habitable-zone Earth-sized Planet Rescued from False Positive Status
DOI: 10.3847/2041-8213/ab84e5 Bibcode: 2020ApJ...893L..27V

Vanderburg, Andrew; Bryson, Steve; Latham, David W. +9 more

We report the discovery of an Earth-sized planet in the habitable zone of a low-mass star called Kepler-1649. The planet, Kepler-1649 c, is 1.06 ${}_{-0.10}^{+0.15}$ times the size of Earth and transits its 0.1977 ± 0.0051 ${M}_{\odot }$ "mid" M-dwarf host star every 19.5 days. It receives 74% ± 3% the incident flux of Earth, giving it an equilibr…

2020 The Astrophysical Journal
Gaia 17