Search Publications

Confirming Herschel Candidate Protoclusters from ALMA/VLA CO Observations
DOI: 10.3847/1538-4357/ab002a Bibcode: 2019ApJ...872..117G

Pérez-Fournon, I.; Valtchanov, I.; Clements, D. L. +11 more

ALMA 870 µm continuum imaging has uncovered a population of blends of multiple dusty star-forming galaxies (DSFGs) in sources originally detected with the Herschel Space Observatory. However, their pairwise separations are much smaller than what is found by ALMA follow-up of other single-dish surveys or expected from theoretical simulations.…

2019 The Astrophysical Journal
Herschel 58
Weighing the Darkness: Astrometric Mass Measurement of Hidden Stellar Companions Using Gaia
DOI: 10.3847/1538-4357/ab441f Bibcode: 2019ApJ...886...68A

Breivik, Katelyn; Andrews, Jeff J.; Chatterjee, Sourav

In astrometric binaries, the presence of a dark, unseen star can be inferred from the gravitational pull it induces on its luminous binary companion. While the orbit of such binaries can be characterized with precise astrometric measurements, constraints made from astrometry alone are not enough to measure the component masses. In this work, we de…

2019 The Astrophysical Journal
Gaia 58
Discovery of Highly Blueshifted Broad Balmer and Metastable Helium Absorption Lines in a Tidal Disruption Event
DOI: 10.3847/1538-4357/ab24de Bibcode: 2019ApJ...879..119H

Cenko, S. B.; Veilleux, S.; Foley, Ryan J. +25 more

We report the discovery of nonstellar hydrogen Balmer and metastable helium absorption lines accompanying a transient, high-velocity (0.05c) broad absorption line (BAL) system in the optical spectra of the tidal disruption event (TDE) AT2018zr (z = 0.071). In the Hubble Space Telescope UV spectra, absorption of high- and low-ionization lines is al…

2019 The Astrophysical Journal
eHST 58
Slowing of the Solar Wind in the Outer Heliosphere
DOI: 10.3847/1538-4357/ab3e49 Bibcode: 2019ApJ...885..156E

Stern, S. Alan; Weaver, Harold A.; Young, Leslie A. +15 more

This study provides a deeper understanding of how the solar wind evolves with increasing distance from the Sun as it encounters an increasing amount of interstellar material. This work extends our prior work by (1) extending the solar wind proton data radial profiles for New Horizons (NH) out to nearly 43 au, (2) quantifying the observed amount of…

2019 The Astrophysical Journal
Ulysses 57
The Main Sequence at z ∼ 1.3 Contains a Sizable Fraction of Galaxies with Compact Star Formation Sizes: A New Population of Early Post-starbursts?
DOI: 10.3847/2041-8213/ab1f92 Bibcode: 2019ApJ...877L..23P

Daddi, E.; Elbaz, D.; Le Floc'h, E. +20 more

Atacama Large Millimeter/submillimeter Array (ALMA) measurements for 93 Herschel-selected galaxies at 1.1 ≤ z ≤ 1.7 in COSMOS reveal a sizable (>29%) population with compact star formation (SF) sizes, lying on average >×3.6 below the optical stellar mass (M )-size relation of disks. This sample widely spans the star-forming main …

2019 The Astrophysical Journal
Herschel 57
Flaring Activity of Proxima Centauri from TESS Observations: Quasiperiodic Oscillations during Flare Decay and Inferences on the Habitability of Proxima b
DOI: 10.3847/1538-4357/ab41f5 Bibcode: 2019ApJ...884..160V

Pál, András; Moór, Attila; Vida, Krisztián +3 more

We analyze the light curve of the M5.5 dwarf Proxima Centauri obtained by the Transiting Exoplanet Survey Satellite (TESS) in Sectors 11 and 12. In the ≈50 day long light curve we identified and analyzed 72 flare events. The flare rate was 1.49 events per day; in total, 7.2% of the observing time was classified as flaring. The estimated flare ener…

2019 The Astrophysical Journal
Gaia 57
Back to the Lithium Plateau with the [Fe/H] < -6 Star J0023+0307
DOI: 10.3847/2041-8213/ab1076 Bibcode: 2019ApJ...874L..21A

Aguado, David S.; Allende Prieto, Carlos; Rebolo, Rafael +1 more

We present an analysis of the Ultraviolet and Visual Echelle Spectrograph (UVES) high-resolution spectroscopic observations at the 8.2 m Very Large Telescope of J0023+0307, a main-sequence extremely iron-poor dwarf star. We are unable to detect iron lines in the spectrum but derive [Fe/H] < -6.1 from the Ca II resonance lines assuming [Ca/Fe] ≥…

2019 The Astrophysical Journal
Gaia 56
The SPIRITS Sample of Luminous Infrared Transients: Uncovering Hidden Supernovae and Dusty Stellar Outbursts in Nearby Galaxies
DOI: 10.3847/1538-4357/ab4a01 Bibcode: 2019ApJ...886...40J

Williams, Robert E.; Kilpatrick, Charles D.; Tinyanont, Samaporn +23 more

We present a systematic study of the most luminous (M IR [Vega magnitudes] brighter than -14) infrared (IR) transients discovered by the SPitzer InfraRed Intensive Transients Survey (SPIRITS) between 2014 and 2018 in nearby galaxies (D < 35 Mpc). The sample consists of nine events that span peak IR luminosities of M [4.5],peak

2019 The Astrophysical Journal
eHST 56
The COS CGM Compendium. II. Metallicities of the Partial and Lyman Limit Systems at z ≲ 1
DOI: 10.3847/1538-4357/aafb74 Bibcode: 2019ApJ...872...81W

Lehner, Nicolas; Howk, J. Christopher; O'Meara, John M. +3 more

We present the results from our COS circumgalactic medium (CGM) compendium (CCC), a survey of the CGM at z ≲ 1 using H I-selected absorbers with 15 < {log}{N}{{H}{{I}}} < 19. We focus here on 82 partial Lyman limit systems (pLLSs, 16.2 ≤ {log}{N}{{H}{{I}}} < 17.2) and 29 LLSs (17.2 ≤ {log}{N}{{H}{{I}}} <…

2019 The Astrophysical Journal
eHST 56
Evidence for Sub-Chandrasekhar Type Ia Supernovae from Stellar Abundances in Dwarf Galaxies
DOI: 10.3847/1538-4357/ab2c02 Bibcode: 2019ApJ...881...45K

Kovalev, Mikhail; McWilliam, Andrew; Shen, Ken J. +6 more

There is no consensus on the progenitors of Type Ia supernovae (SNe Ia) despite their importance for cosmology and chemical evolution. We address this question using our previously published catalogs of Mg, Si, Ca, Cr, Fe, Co, and Ni abundances in dwarf galaxy satellites of the Milky Way (MW) to constrain the mass at which the white dwarf (WD) exp…

2019 The Astrophysical Journal
Gaia 56