Search Publications

Dynamical Masses for the Hyades Binary 80 Tauri
DOI: 10.3847/1538-4357/ab3a30 Bibcode: 2019ApJ...883..105T

Torres, Guillermo

The empirical mass-luminosity relation in the Hyades cluster rests on dynamical mass determinations for five binary systems, of which one is eclipsing and the other four are visual or interferometric binaries. The last one was identified and first measured more than 20 yr ago. Here we present dynamical mass measurements for a new binary system in …

2019 The Astrophysical Journal
Gaia Hipparcos 10
Active Galactic Nuclei in Dusty Starbursts at z = 2: Feedback Still to Kick in
DOI: 10.3847/2041-8213/ab222e Bibcode: 2019ApJ...877L..38R

Daddi, E.; Rodighiero, G.; Rujopakarn, W. +18 more

We investigate a sample of 152 dusty sources at 1.5 < z < 2.5 to understand the connection of enhanced star formation rate (SFR) and black hole accretion rate. The sources are Herschel-selected, having stellar masses M * > 1010 M and SFR (∼100-1000 M yr-1) elevated (>4×) above …

2019 The Astrophysical Journal
Herschel 10
Stellar Pulsation and the Production of Dust and Molecules in Galactic Carbon Stars
DOI: 10.3847/1538-4357/ab4f6b Bibcode: 2019ApJ...887...82K

McDonald, Iain; Sloan, G. C.; Groenewegen, Martin A. T. +3 more

New infrared spectra of 33 Galactic carbon stars from FORCAST on SOFIA reveal strong connections between stellar pulsations and the dust and molecular chemistry in their circumstellar shells. A sharp boundary in overall dust content, which predominantly measures the amount of amorphous carbon, separates the semiregular and Mira variables, with the…

2019 The Astrophysical Journal
ISO 10
The Time-domain Spectroscopic Survey: Radial Velocity Variability in Dwarf Carbon Stars
DOI: 10.3847/1538-4357/ab1a3e Bibcode: 2019ApJ...877...44R

Roulston, Benjamin R.; Green, Paul J.; Anderson, Scott F. +6 more

Dwarf carbon (dC) stars (main-sequence stars showing carbon molecular bands) were initially thought to be an oxymoron because only asymptotic giant branch (AGB) stars dredge carbon into their atmospheres. Mass transfer from a former AGB companion that has since faded to a white dwarf seems the most likely explanation. Indeed, a few types of giants…

2019 The Astrophysical Journal
Gaia 10
On the Relation between Flare and CME during GLE-SEP and Non-GLE-SEP Events
DOI: 10.3847/1538-4357/ab3c4e Bibcode: 2019ApJ...883...91F

Gan, W. Q.; Moon, Y. -J.; Rodríguez-Pacheco, J. +2 more

Association of solar flares and coronal mass ejections (CMEs) with ground-level enhancement (GLE) is a recognized fact, but questions arise when a similar association is observed for non-GLEs. In this respect, we carry out a detailed study of the relation between flare fluences (ϕ J m-2) and CME speeds (V cme km s-1

2019 The Astrophysical Journal
SOHO 9
FUSE Spectroscopic Analysis of the Slowest Symbiotic Nova AG Peg During Quiescence
DOI: 10.3847/1538-4357/ab0c0a Bibcode: 2019ApJ...874..178S

Sion, Edward M.; Godon, Patrick; Mikolajewska, Joanna +1 more

We present a far-UV (FUV) spectroscopic analysis of the slowest known symbiotic nova AG Peg that underwent a nova explosion in 1850 followed by a very slow decline that did not end until ∼1996, marking the beginning of quiescence. In 2015 June, when AG Peg exhibited a Z And-type outburst with an optical amplitude of ∼1.5 mag. We used accretion dis…

2019 The Astrophysical Journal
Gaia 9
The Period Change of Cyg X-3
DOI: 10.3847/1538-4357/aafb38 Bibcode: 2019ApJ...871..244A

Antokhin, Igor I.; Cherepashchuk, Anatol M.

By using available archival X-ray data, we significantly extended the list of times of X-ray minima. The new list includes 65 data points obtained by critically reanalyzing RXTE ASM data, 88 data points based on observations by MAXI, and 2 data points based on observations by SUZAKU and AstroSat. Analyzing the data along with times of X-ray minima…

2019 The Astrophysical Journal
Suzaku 9
Torus Constraints in ANEPD-CXO245: A Compton-thick AGN with Double-peaked Narrow Lines
DOI: 10.3847/2041-8213/ab46bc Bibcode: 2019ApJ...884L..10M

Goto, Tomotsugu; Burgarella, Denis; Tanimoto, Atsushi +18 more

We report on the torus constraints of the Compton-thick active galactic nucleus (AGN) with double-peaked optical narrow-line region emission lines, ANEPD-CXO245, at z = 0.449 in the AKARI NEP Deep Field. The unique infrared data on this field, including those from the nine-band photometry over 2-24 µm with the AKARI Infrared Camera, and the …

2019 The Astrophysical Journal
AKARI 9
Properties of the Diffuse Emission around Warm Loops in Solar Active Regions
DOI: 10.3847/1538-4357/ab0179 Bibcode: 2019ApJ...873...26B

Brooks, David H.

Coronal loops in active regions are the subjects of intensive investigation, but the important diffuse unresolved emission in which they are embedded has received relatively little attention. Here I measure the densities and emission measure (EM) distributions of a sample of background-foreground regions surrounding warm (2 MK) coronal loops, and …

2019 The Astrophysical Journal
Hinode 9
The Eruption of Outer Spine-like Loops Leading to a Double-stage Circular-ribbon Flare
DOI: 10.3847/1538-4357/ab3923 Bibcode: 2019ApJ...883...47L

Liu, Chang; Wang, Haimin; Lee, Jeongwoo

Circular-ribbon flares occur in a confined magnetic structure, but can also be associated with coronal mass ejections (CMEs) when a filament embedded under the fan erupts. Here we study an M8.7 circular-ribbon flare (SOL2014-12-17T04:51), which is accompanied by a CME yet without a clear indication of filament eruption. Using a nonlinear force-fre…

2019 The Astrophysical Journal
SOHO 9