Search Publications

The Luminosity Function of Red Supergiants in M31
DOI: 10.3847/1538-4357/ab5ba0 Bibcode: 2020ApJ...889...44N

Drout, Maria R.; Massey, Philip; Levesque, Emily M. +5 more

The mass-loss rates of red supergiant stars (RSGs) are poorly constrained by direct measurements, and yet the subsequent evolution of these stars depends critically on how much mass is lost during the RSG phase. In 2012 the Geneva evolutionary group updated their mass-loss prescription for RSGs with the result that a 20 M star now lose…

2020 The Astrophysical Journal
Gaia 32
Narrowband Large Amplitude Whistler-mode Waves in the Solar Wind and Their Association with Electrons: STEREO Waveform Capture Observations
DOI: 10.3847/1538-4357/ab961f Bibcode: 2020ApJ...897..126C

Breneman, A. W.; Cattell, C. A.; Short, B. +1 more

Large amplitude (up to 70 mV m-1) whistler-mode waves at frequencies of ∼0.2-0.4 fce (electron cyclotron frequency) are frequently observed in the solar wind. The waves are obliquely propagating at angles close to the resonance cone, resulting in significant electric fields parallel to the background magnetic field, enabling …

2020 The Astrophysical Journal
Cluster 32
Supernovae in Orion: The Missing Link in the Star-forming History of the Region
DOI: 10.3847/1538-4357/abb6e8 Bibcode: 2020ApJ...902..122K

Kounkel, Marina

The Orion Complex is a notable star-forming region fragmented into several different populations with substantial differences in their phase space. I propose a model that attempts to explain the how the Complex has evolved into this current configuration. In the model presented here, the large-scale expansion can be attributable to a supernova tha…

2020 The Astrophysical Journal
Gaia 32
The Morphology-Density Relationship in 1 < z < 2 Clusters
DOI: 10.3847/1538-4357/aba42f Bibcode: 2020ApJ...899...85S

Rodriguez-Gomez, Vicente; Snyder, Gregory F.; Brodwin, Mark +8 more

The morphology-density relationship states that dense cosmic environments such as galaxy clusters have an overabundance of quiescent elliptical galaxies, but it is unclear at which redshift this relationship is first established. We study the morphology of four clusters with 1.2 < z < 1.8 using Hubble Space Telescope imaging and the morpholo…

2020 The Astrophysical Journal
eHST 32
An Isolated White Dwarf with 317 s Rotation and Magnetic Emission
DOI: 10.3847/1538-4357/ab8239 Bibcode: 2020ApJ...894...19R

Hermes, J. J.; Clemens, J. C.; Vanderbosch, Z. +5 more

We report the discovery of short-period photometric variability and modulated Zeeman-split hydrogen emission in SDSSJ125230.93-023417.72 (EPIC 228939929), a variable white dwarf star observed at long cadence in K2 Campaign 10. The behavior is associated with a magnetic (B = 5.0 MG) spot on the stellar surface, making the 317.278 s period a direct …

2020 The Astrophysical Journal
Gaia 32
Blazars at the Cosmic Dawn
DOI: 10.3847/1538-4357/ab9c1a Bibcode: 2020ApJ...897..177P

Ajello, M.; Giroletti, M.; Madejski, Greg +5 more

The uncharted territory of the high-redshift (z ≳ 3) universe holds the key to understanding the evolution of quasars. In an attempt to identify the most extreme members of the quasar population, that is, blazars, we have carried out a multiwavelength study of a large sample of radio-loud quasars beyond z = 3. Our sample consists of nine γ-ray-det…

2020 The Astrophysical Journal
XMM-Newton 32
A Kinematic View of NGC 1261: Structural Parameters, Internal Dispersion, Absolute Proper Motion, and Blue Straggler Stars
DOI: 10.3847/1538-4357/ab8ae7 Bibcode: 2020ApJ...895...15R

Anderson, Jay; Cadelano, Mario; Pallanca, Cristina +8 more

We constructed a Hubble Space Telescope (HST) astrophotometric catalog of the central region of the Galactic globular cluster NGC 1261. This catalog, complemented with Gaia DR2 data sampling the external regions, has been used to estimate the structural parameters of the system (I.e., core, half-mass, tidal radii, and concentration) from its resol…

2020 The Astrophysical Journal
Gaia eHST 32
Infrared Excesses around Bright White Dwarfs from Gaia and unWISE. I.
DOI: 10.3847/1538-4357/abb3fc Bibcode: 2020ApJ...902..127X

Lai, Samuel; Xu, Siyi; Dennihy, Erik

Studies of excess infrared radiation around white dwarfs provide important constraints on the evolution of planetary systems and low-mass companions beyond the main-sequence stage. In this paper series, we focus on identifying and characterizing bright white dwarfs with an infrared excess. Here, we present 188 infrared excess candidates from Gaia …

2020 The Astrophysical Journal
Gaia 32
Direct Radio Discovery of a Cold Brown Dwarf
DOI: 10.3847/2041-8213/abc256 Bibcode: 2020ApJ...903L..33V

Callingham, J. R.; Shimwell, T. W.; Vedantham, H. K. +9 more

Magnetospheric processes seen in gas giants such as aurorae and circularly polarized cyclotron maser radio emission have been detected from some brown dwarfs. However, previous radio observations targeted known brown dwarfs discovered via their infrared emission. Here we report the discovery of BDR J1750+3809, a circularly polarized radio source d…

2020 The Astrophysical Journal
Gaia 32
The Angular Momentum of the Circumgalactic Medium in the TNG100 Simulation
DOI: 10.3847/1538-4357/ab8a4a Bibcode: 2020ApJ...895...17D

Genel, Shy; Pillepich, Annalisa; Nelson, Dylan +3 more

We present an analysis of the angular momentum content of the circumgalactic medium (CGM) using TNG100, one of the flagship runs of the IllustrisTNG project. We focus on Milky Way-mass halos (∼1012 M) at z = 0 but also analyze other masses and redshifts up to z = 5. We find that the CGM angular momentum properties are strong…

2020 The Astrophysical Journal
eHST 32