Search Publications

The Strength of the 2175 Å Feature in the Attenuation Curves of Galaxies at 0.1 < z ≲ 3
DOI: 10.3847/1538-4357/ab5fdd Bibcode: 2020ApJ...888..108B

Calzetti, D.; Battisti, A. J.; Cunha, E. da +1 more

We update the spectral modeling code MAGPHYS to include a 2175 Å absorption feature in its UV to near-IR dust attenuation prescription. This allows us to determine the strength of this feature and the shape of the dust attenuation curve in ∼5000 star-forming galaxies at $0.1\lt z\lesssim 3$ in the COSMOS field. We find that a 2175 Å absorption fea…

2020 The Astrophysical Journal
eHST 39
Astrophysical Distance Scale: The AGB J-band Method. I. Calibration and a First Application
DOI: 10.3847/1538-4357/aba045 Bibcode: 2020ApJ...899...66M

Madore, Barry F.; Freedman, Wendy L.

A near-infrared, color-selected subset of carbon-rich asymptotic giant branch (C-AGB) stars is found to have tightly constrained luminosities in the near-infrared J band. Based on JK photometry of some 3300 C-AGB stars in the bar of the Large Magellanic Cloud (LMC) we find that these stars have a constant absolute magnitude of $\langle {M}_{J}\ran…

2020 The Astrophysical Journal
eHST 39
The Complex Space Weather Events of 2017 September
DOI: 10.3847/1538-4357/aba2c5 Bibcode: 2020ApJ...899....3H

Hajra, Rajkumar; Tsurutani, Bruce T.; Lakhina, Gurbax S.

Interplanetary coronal mass ejections (ICMEs), magnetic clouds (MCs), sheaths, corotating interaction regions (CIRs), solar wind high-speed streams (HSSs), fast forward shocks (FSs), reverse waves (RWs), stream interfaces, and heliospheric current sheet crossings detected upstream of the Earth and their geoeffectiveness are studied during 2017 Sep…

2020 The Astrophysical Journal
SOHO 39
Dual-wavelength ALMA Observations of Dust Rings in Protoplanetary Disks
DOI: 10.3847/1538-4357/ab9a54 Bibcode: 2020ApJ...898...36L

Pascucci, Ilaria; Herczeg, Gregory J.; Wilner, David J. +13 more

We present new Atacama Large Millimeter/submillimeter Array observations for three protoplanetary disks in Taurus at 2.9 mm and comparisons with previous 1.3 mm data both at an angular resolution of ∼0"1 (15 au for the distance of Taurus). In the single-ring disk DS Tau, double-ring disk GO Tau, and multiring disk DL Tau, the same rings are detect…

2020 The Astrophysical Journal
Gaia 39
The young massive SMC cluster NGC 330 seen by MUSE. I. Observations and stellar content
DOI: 10.1051/0004-6361/201936743 Bibcode: 2020A&A...634A..51B

Lennon, D. J.; de Mink, S. E.; de Koter, A. +9 more

Context. A majority of massive stars are part of binary systems, a large fraction of which will inevitably interact during their lives. Binary-interaction products (BiPs), that is, stars affected by such interaction, are expected to be commonly present in stellar populations. BiPs are thus a crucial ingredient in the understanding of stellar evolu…

2020 Astronomy and Astrophysics
Gaia eHST 39
Full of Orions: a 200-pc mapping of the interstellar medium in the redshift-3 lensed dusty star-forming galaxy SDP.81
DOI: 10.1093/mnras/staa879 Bibcode: 2020MNRAS.494.5542R

Andreani, P.; Vegetti, S.; McKean, J. P. +4 more

We present a sub-kpc resolved study of the interstellar medium properties in SDP.81, a $z$ = 3.042 strongly gravitationally lensed, dusty star-forming galaxy, based on high-resolution, multiband ALMA observations of the far-infrared (FIR) continuum, CO ladder, and the [C II] line. Using a visibility-plane lens modelling code, we achieve a median s…

2020 Monthly Notices of the Royal Astronomical Society
Herschel 39
A Comparison of Flare Forecasting Methods. IV. Evaluating Consecutive-day Forecasting Patterns
DOI: 10.3847/1538-4357/ab65f0 Bibcode: 2020ApJ...890..124P

Leka, K. D.; Gallagher, Peter T.; Murray, Sophie A. +21 more

A crucial challenge to successful flare prediction is forecasting periods that transition between "flare-quiet" and "flare-active." Building on earlier studies in this series in which we describe the methodology, details, and results of flare forecasting comparison efforts, we focus here on patterns of forecast outcomes (success and failure) over …

2020 The Astrophysical Journal
PROBA-2 39
A Blueprint for the Milky Way's Stellar Populations: The Power of Large Photometric and Astrometric Surveys
DOI: 10.3847/1538-4357/ab8d39 Bibcode: 2020ApJ...897...39A

Beers, Timothy C.; An, Deokkeun

Recent advances from astronomical surveys have revealed spatial, chemical, and kinematical inhomogeneities in the inner region of the stellar halo of the Milky Way. In particular, large spectroscopic surveys, combined with Gaia astrometric data, have provided powerful tools for analyzing the detailed abundances and accurate kinematics for individu…

2020 The Astrophysical Journal
Gaia 39
Persistent Starspot Signals on M Dwarfs: Multiwavelength Doppler Observations with the Habitable-zone Planet Finder and Keck/HIRES
DOI: 10.3847/1538-4357/ab989f Bibcode: 2020ApJ...897..125R

Cochran, William D.; Endl, Michael; Mahadevan, Suvrath +23 more

Young, rapidly rotating M dwarfs exhibit prominent starspots, which create quasiperiodic signals in their photometric and Doppler spectroscopic measurements. The periodic Doppler signals can mimic radial velocity (RV) changes expected from orbiting exoplanets. Exoplanets can be distinguished from activity-induced false positives by the chromaticit…

2020 The Astrophysical Journal
Gaia 39
Determination of the Local Hubble Constant from Virgo Infall Using TRGB Distances
DOI: 10.3847/1538-4357/abbd97 Bibcode: 2020ApJ...905..104K

Lee, Myung Gyoon; Kang, Jisu; Jang, In Sung +1 more

An independent determination of H0 is crucial given the growing tension between the Hubble constant, H0, derived locally and that determined from the modeling of the cosmic microwave background (CMB) originating in the early universe. In this work, we present a new determination of H0 using velocities and tip of th…

2020 The Astrophysical Journal
eHST 39