Search Publications

Fragmentation of star-forming filaments in the X-shaped nebula of the California molecular cloud
DOI: 10.1051/0004-6361/202037721 Bibcode: 2020A&A...642A..76Z

André, Ph.; Men'shchikov, A.; Wang, Ke +1 more

Context. Dense molecular filaments are central to the star formation process, but the detailed manner in which they fragment into prestellar cores is not well understood yet.
Aims: Here, we investigate the fragmentation properties and dynamical state of several star-forming filaments in the X-shaped nebula region of the California molecular c…

2020 Astronomy and Astrophysics
Gaia Herschel 29
The Open Universe VOU-Blazars tool
DOI: 10.1016/j.ascom.2019.100350 Bibcode: 2020A&C....3000350C

Giommi, P.; Chang, Y. -L.; Brandt, C. H.

Blazars are a remarkable type of Active Galactic Nuclei (AGN) that are playing an important and rapidly growing role in today's multi-frequency and multi-messenger astrophysics. In the past several years, blazars have been discovered in relatively large numbers in radio, microwave, X-ray and gamma-ray surveys, and more recently have been associate…

2020 Astronomy and Computing
XMM-Newton 29
Inverse stellar population age gradients of post-starburst galaxies at z = 0.8 with LEGA-C
DOI: 10.1093/mnras/staa1937 Bibcode: 2020MNRAS.497..389D

Bell, Eric F.; D'Eugenio, Francesco; Franx, Marijn +13 more

We use deep, spatially resolved spectroscopy from the Large Early Galaxy Astrophysics Census Survey to study radial variations in the stellar population of 17 spectroscopically selected post-starburst (PSB) galaxies. We use spectral fitting to measure two Lick indices, H δA and Fe 4383 , and find that, on average, PSB galaxies have radi…

2020 Monthly Notices of the Royal Astronomical Society
eHST 29
WIYN Open Cluster Study. LXXXII. Radial-velocity Measurements and Spectroscopic Binary Orbits in the Open Cluster NGC 7789
DOI: 10.3847/1538-3881/abad3b Bibcode: 2020AJ....160..169N

Platais, Imants; Tofflemire, Benjamin M.; Mathieu, Robert D. +4 more

We present an extensive time-series radial-velocity (RV) survey of stars in the rich open cluster NGC 7789 (1.6 Gyr, [Fe/H] = +0.02). The stellar sample lies within an 18' circular radius from the cluster center (10 pc in projection, or about 2 core radii), and includes giants, red clump stars, blue stragglers, red stragglers, sub-subgiants, and m…

2020 The Astronomical Journal
Gaia 29
Discovery of new stellar groups in the Orion complex. Towards a robust unsupervised approach
DOI: 10.1051/0004-6361/201935955 Bibcode: 2020A&A...643A.114C

Alves, João; Adamo, Angela; D'Onghia, Elena +1 more

We test the ability of two unsupervised machine learning algorithms, EnLink and Shared Nearest Neighbor (SNN), to identify stellar groupings in the Orion star-forming complex as an application to the 5D astrometric data from Gaia DR2. The algorithms represent two distinct approaches to limiting user bias when selecting parameter values and evaluat…

2020 Astronomy and Astrophysics
Gaia 29
Spitzer + VLTI-GRAVITY Measure the Lens Mass of a Nearby Microlensing Event
DOI: 10.3847/1538-4357/ab9749 Bibcode: 2020ApJ...897..180Z

Feliz, Dax L.; Zang, Weicheng; Gould, Andrew +26 more

We report the lens mass and distance measurements of the nearby microlensing event TCP J05074264+2447555 (Kojima-1). We measure the microlens parallax vector ${{\boldsymbol{\pi }}}_{{\rm{E}}}$ using Spitzer and ground-based light curves with constraints on the direction of lens-source relative proper motion derived from Very Large Telescope Interf…

2020 The Astrophysical Journal
Gaia 29
Hunting for Runaways from the Orion Nebula Cluster
DOI: 10.3847/1538-4357/aba699 Bibcode: 2020ApJ...900...14F

Tan, Jonathan C.; Eyer, Laurent; Farias, Juan P.

We use Gaia DR2 to hunt for runaway stars from the Orion Nebula Cluster (ONC). We search a region extending 45° around the ONC and out to 1 kpc to find sources that have overlapped in angular position with the cluster in the last ∼10 Myr. We find ∼17,000 runaway/walkaway candidates that satisfy this 2D traceback condition. Most of these are expect…

2020 The Astrophysical Journal
Gaia 29
The Fornax 3D project: Globular clusters tracing kinematics and metallicities
DOI: 10.1051/0004-6361/202037685 Bibcode: 2020A&A...637A..26F

Viaene, S.; Hilker, M.; Pinna, F. +15 more

Globular clusters (GCs) are found ubiquitously in massive galaxies and due to their old ages, they are regarded as fossil records of galaxy evolution. Spectroscopic studies of GC systems are often limited to the outskirts of galaxies, where GCs stand out against the galaxy background and serve as bright tracers of galaxy assembly. In this work, we…

2020 Astronomy and Astrophysics
eHST 29
The Gaia-ESO Survey: detection and characterisation of single-line spectroscopic binaries
DOI: 10.1051/0004-6361/201935819 Bibcode: 2020A&A...635A.155M

Gilmore, G.; Bayo, A.; Mowlavi, N. +26 more

Context. Multiple stellar systems play a fundamental role in the formation and evolution of stellar populations in galaxies. Recent and ongoing large ground-based multi-object spectroscopic surveys significantly increase the sample of spectroscopic binaries (SBs) allowing analyses of their statistical properties.
Aims: We investigate the repe…

2020 Astronomy and Astrophysics
Gaia 29
Unsupervised machine learning for transient discovery in deeper, wider, faster light curves
DOI: 10.1093/mnras/staa2395 Bibcode: 2020MNRAS.498.3077W

Andreoni, Igor; Mahabal, Ashish; Cooke, Jeff +7 more

Identification of anomalous light curves within time-domain surveys is often challenging. In addition, with the growing number of wide-field surveys and the volume of data produced exceeding astronomers' ability for manual evaluation, outlier and anomaly detection is becoming vital for transient science. We present an unsupervised method for trans…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 29