Search Publications

Three new Galactic star clusters discovered in the field of the open cluster NGC 5999 with Gaia DR2
DOI: 10.1093/mnras/sty3511 Bibcode: 2019MNRAS.483.5508F

Corradi, W. J. B.; Ferreira, Filipe A.; Santos, J. F. C. +2 more

We report the serendipitous discovery of three new open clusters, named UFMG 1, UFMG 2, and UFMG 3 in the field of the intermediate-age cluster NGC 5999, by using Gaia DR2 data. A colour-magnitude filter tailored for a proper selection of main-sequence stars and red clump giants turned evident the presence of NGC 5999 and these three new stellar g…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 39
Molecular complexity on disc scales uncovered by ALMA. Chemical composition of the high-mass protostar AFGL 4176
DOI: 10.1051/0004-6361/201834527 Bibcode: 2019A&A...628A...2B

van Dishoeck, Ewine F.; Hogerheijde, Michiel R.; Ligterink, Niels F. W. +4 more

Context. The chemical composition of high-mass protostars reflects the physical evolution associated with different stages of star formation. In addition, the spatial distribution and velocity structure of different molecular species provide valuable information on the physical structure of these embedded objects. Despite an increasing number of i…

2019 Astronomy and Astrophysics
Gaia 39
The white dwarf mass-radius relation and its dependence on the hydrogen envelope
DOI: 10.1093/mnras/stz160 Bibcode: 2019MNRAS.484.2711R

Kepler, S. O.; Romero, Alejandra D.; Joyce, S. R. G. +2 more

We present a study of the dependence of the mass-radius relation for DA white dwarf stars on the hydrogen envelope mass and the impact on the value of log g, and thus the determination of the stellar mass. We employ a set of full evolutionary carbon-oxygen core white dwarf sequences with white dwarf mass between 0.493 and 1.05 M. Compu…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 38
Infrared Contributions of X-Ray Selected Active Galactic Nuclei in Dusty Star-forming Galaxies
DOI: 10.3847/1538-4357/aaf73b Bibcode: 2019ApJ...871...87B

Azadi, Mojegan; Cooray, Asantha; Ma, Jingzhe +3 more

We investigate the infrared (IR) contribution from supermassive black hole activity versus host galaxy emission in the mid- to far-IR spectrum for a large sample of X-ray bright active galactic nuclei (AGN) residing in dusty, star-forming host galaxies. We select 703 AGN with {L}{{X}}={10}42{--}{10}46 erg s-1<…

2019 The Astrophysical Journal
Herschel 38
SWAN/SOHO Lyman-α Mapping: The Hydrogen Geocorona Extends Well Beyond the Moon
DOI: 10.1029/2018JA026136 Bibcode: 2019JGRA..124..861B

Schmidt, W.; Bertaux, J. -L.; Quémerais, E. +2 more

The Earth's hydrogen exosphere Lyman-α radiation was mapped with the Solar Wind Anisotropies/Solar and Heliospheric Observatory (SWAN/SOHO) instrument in January 1996, 1997, and 1998 (low solar activity). The use of a hydrogen absorption cell allowed to disentangle the interplanetary emission from the geocoronal one and to assign the absorbed sign…

2019 Journal of Geophysical Research (Space Physics)
SOHO 38
A stellar relic filament in the Orion star-forming region
DOI: 10.1093/mnras/stz2315 Bibcode: 2019MNRAS.489.4418J

Anderson, Richard I.; Boffin, Henri M. J.; Jerabkova, Tereza +1 more

We report the discovery of the oldest stellar substructure in the Orion star-forming region (OSFR), the Orion relic filament. The relic filament is physically associated with the OSFR, as demonstrated by Gaia DR2 photometry and astrometry, as well as by targeted radial velocity follow-up observations of a bright subsample of proper motion-selected…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 38
First ALMA Millimeter-wavelength Maps of Jupiter, with a Multiwavelength Study of Convection
DOI: 10.3847/1538-3881/ab3643 Bibcode: 2019AJ....158..139D

de Pater, Imke; Sault, R. J.; Wong, Michael H. +15 more

We obtained the first maps of Jupiter at 1-3 mm wavelength with the Atacama Large Millimeter/Submillimeter Array (ALMA) on 2017 January 3-5, just days after an energetic eruption at 16.°5S jovigraphic latitude had been reported by the amateur community, and about two to three months after the detection of similarly energetic eruptions in the north…

2019 The Astronomical Journal
eHST 38
Detection of a 50° long Trailing Tidal Tail for the Globular Cluster M5
DOI: 10.3847/1538-4357/ab441d Bibcode: 2019ApJ...884..174G

Grillmair, Carl J.

Using photometry and proper motions from Gaia Data Release 2, we detect a 50° long stream of about 70 stars extending westward from the halo globular cluster M5. Based on the similarities in distance, proper motions, inferred color-magnitude distribution, and trajectory, we identify this stream as the trailing tidal tail of M5. While the surface d…

2019 The Astrophysical Journal
Gaia 38
HST unveils a compact mildly relativistic broad-line region in the candidate true type 2 NGC 3147
DOI: 10.1093/mnrasl/slz080 Bibcode: 2019MNRAS.488L...1B

Laor, Ari; Bianchi, Stefano; La Franca, Fabio +9 more

NGC 3147 has been considered the best case of a true type 2 AGN: an unobscured AGN, based on the unabsorbed compact X-ray continuum, which lacks a broad-line region (BLR). However, the very low luminosity of NGC 3147 implies a compact BLR, which produces very broad lines, hard to detect against the dominant background host galaxy. Narrow (0.1 arcs…

2019 Monthly Notices of the Royal Astronomical Society
eHST 38
Episodically Active Asteroid 6478 Gault
DOI: 10.3847/2041-8213/ab1be8 Bibcode: 2019ApJ...876L..19J

Kotulla, Ralf; Jewitt, David; Rajagopal, Jayadev +4 more

We present imaging and spectroscopic observations of 6478 Gault, a ∼6 km diameter inner main-belt asteroid currently exhibiting strong, comet-like characteristics. Three distinct tails indicate that ultra-slow dust (ejection speed 0.15 ± 0.05 m s-1) was emitted from Gault in separate episodes beginning UT 2018 October 28 ± 5 (Tail A), U…

2019 The Astrophysical Journal
eHST 38