Search Publications

Wide Twin Binaries are Extremely Eccentric: Evidence of Twin Binary Formation in Circumbinary Disks
DOI: 10.3847/2041-8213/ac7c70 Bibcode: 2022ApJ...933L..32H

Ting, Yuan-Sen; Rix, Hans-Walter; Zakamska, Nadia L. +3 more

The Gaia mission recently revealed an excess population of equal-mass "twin" wide binaries, with mass ratio q ≳ 0.95, extending to separations of at least 1000 au. The origin of this population is an enigma: Twin binaries are thought to form via correlated accretion in circumbinary disks, but the typical observed protostellar disks have radii of ~…

2022 The Astrophysical Journal
Gaia 22
An INTEGRAL/SPI view of reticulum II: particle dark matter and primordial black holes limits in the MeV range
DOI: 10.1093/mnras/stac008 Bibcode: 2022MNRAS.511..914S

Calore, Francesca; Vincent, Aaron C.; Diehl, Roland +4 more

Reticulum II (Ret II) is a satellite galaxy of the Milky Way (MW) and presents a prime target to investigate the nature of dark matter (DM) because of its high mass-to-light ratio. We evaluate a dedicated INTEGRAL observation campaign data set to obtain γ-ray fluxes from Ret II and compare those with expectations from DM. Ret II is not detected in…

2022 Monthly Notices of the Royal Astronomical Society
INTEGRAL 22
Contribution of Gaia Sausage to the Galactic Stellar Halo Revealed by K Giants and Blue Horizontal Branch Stars from the Large Sky Area Multi-Object Fiber Spectroscopic Telescope, Sloan Digital Sky Survey, and Gaia
DOI: 10.3847/1538-4357/ac31ac Bibcode: 2022ApJ...924...23W

Bird, Sarah A.; Zhao, Gang; Yang, Chengqun +2 more

We explore the contribution of the Gaia Sausage to the stellar halo of the Milky Way by making use of a Gaussian mixture model (GMM) and applying it to halo star samples of Large Sky Area Multi-Object Fiber Spectroscopic Telescope K giants, Sloan Extension for Galactic Understanding and Exploration K giants, and Sloan Digital Sky Survey blue horiz…

2022 The Astrophysical Journal
Gaia 22
The XMM Cluster Survey analysis of the SDSS DR8 redMaPPer catalogue: implications for scatter, selection bias, and isotropy in cluster scaling relations
DOI: 10.1093/mnras/stac2414 Bibcode: 2022MNRAS.516.3878G

Nichol, R. C.; Miller, C. J.; Romer, A. K. +21 more

In this paper, we present the X-ray analysis of Sloan Digital Sky Survey DR8 redMaPPer (SDSSRM) clusters using data products from the XMM Cluster Survey (XCS). In total, 1189 SDSSRM clusters fall within the XMM-Newton footprint. This has yielded 456 confirmed detections accompanied by X-ray luminosity (LX) measurements. Of these cluster…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 22
New binaries from the SHINE survey
DOI: 10.1051/0004-6361/202140510 Bibcode: 2022A&A...663A.144B

Moutou, C.; Rouan, D.; Avenhaus, H. +68 more

We present the multiple stellar systems observed within the SpHere INfrared survey for Exoplanet (SHINE). SHINE searched for sub-stellar companions to young stars using high contrast imaging. Although stars with known stellar companions within the SPHERE field of view (< 5.5 arcsec) were removed from the original target list, we detected additi…

2022 Astronomy and Astrophysics
AKARI Gaia 22
Deep images of the Galactic center with GRAVITY
DOI: 10.1051/0004-6361/202142459 Bibcode: 2022A&A...657A..82G

Lutz, D.; Förster Schreiber, N. M.; Genzel, R. +65 more

Stellar orbits at the Galactic Center provide a very clean probe of the gravitational potential of the supermassive black hole. They can be studied with unique precision, beyond the confusion limit of a single telescope, with the near-infrared interferometer GRAVITY. Imaging is essential to search the field for faint, unknown stars on short orbits…

2022 Astronomy and Astrophysics
Gaia 22
Dissecting the Different Components of the Modest Accretion Bursts of the Very Young Protostar HOPS 373
DOI: 10.3847/1538-4357/ac5632 Bibcode: 2022ApJ...929...60Y

Herczeg, Gregory J.; Manoj, P.; Johnstone, Doug +11 more

Observed changes in protostellar brightness can be complicated to interpret. In our James Clerk Maxwell Telescope (JCMT) Transient Monitoring Survey, we discovered that a young binary protostar, HOPS 373, is undergoing a modest 30% brightness increase at 850 µm, caused by a factor of 1.8-3.3 enhancement in the accretion rate. The initial bur…

2022 The Astrophysical Journal
Gaia Herschel 22
A 38 Million Year Old Neptune-sized Planet in the Kepler Field
DOI: 10.3847/1538-3881/ac4966 Bibcode: 2022AJ....163..121B

Tamura, M.; Narita, N.; Bouma, L. G. +12 more

Kepler 1627A is a G8V star previously known to host a 3.8 R planet on a 7.2 day orbit. The star was observed by the Kepler space telescope because it is nearby (d = 329 pc) and it resembles the Sun. Here, we show using Gaia kinematics, TESS stellar rotation periods, and spectroscopic lithium abundances that Kepler 1627 is a member of …

2022 The Astronomical Journal
Gaia 22
Searching Far and Long. I. Pilot ALMA 2 mm Follow-up of Bright Dusty Galaxies as a Redshift Filter
DOI: 10.3847/1538-4357/ac616d Bibcode: 2022ApJ...930...32C

Casey, Caitlin M.; Long, Arianna S.; Zavala, Jorge A. +5 more

A complete census of dusty star-forming galaxies (DSFGs) at early epochs is necessary to constrain the obscured contribution to the cosmic star formation rate density (CSFRD); however, DSFGs beyond z ~ 4 are both rare and hard to identify from photometric data alone due to degeneracies in submillimeter photometry with redshift. Here, we present a …

2022 The Astrophysical Journal
Herschel 22
On the Stability of Tidal Streams in Action Space
DOI: 10.3847/1538-4357/ac93fb Bibcode: 2022ApJ...939....2A

Wetzel, Andrew; Cunningham, Emily C.; Sanderson, Robyn E. +3 more

In the Gaia era it is increasingly apparent that traditional static, parameterized models are insufficient to describe the mass distribution of our complex, dynamically evolving Milky Way (MW). In this work, we compare different time-evolving and time-independent representations of the gravitational potentials of simulated MW-mass galaxies from th…

2022 The Astrophysical Journal
Gaia 22