Search Publications

Size Scaling of Clump Instabilities in Turbulent, Feedback-regulated Disks
DOI: 10.3847/1538-4357/ab0b41 Bibcode: 2019ApJ...874..170A

Glazebrook, Karl; Fisher, Deanne B.; Obreschkow, Danail +5 more

We explore the scaling between the size of star-forming clumps and rotational support in massively star-forming galactic disks. The analysis relies on simulations of a clumpy galaxy at z = 2 and the observed DYnamics of Newly Assembled Massive Objects (DYNAMO) sample of rare clumpy analogs at z ≈ 0.1 to test a predictive clump size scaling propose…

2019 The Astrophysical Journal
eHST 0
Silicate features in the circumstellar envelopes of the Class I binary driving source of HH 250
DOI: 10.1051/0004-6361/201834743 Bibcode: 2019A&A...628A..97C

Comerón, F.; Merín, B.; Reipurth, B. +1 more

Context. The silicate feature near 10 µm is one of the main tools available to study the mineralogy of circumstellar disks and envelopes, providing information on the thermal processing, growth, location, and circulation of dust grains.
Aims: We investigate the silicate feature of the two Class I components of HH 250-IRS, a resolved bin…

2019 Astronomy and Astrophysics
Gaia 0
Publisher Correction: Martian dust storm impact on atmospheric H2O and D/H observed by ExoMars Trace Gas Orbiter
DOI: 10.1038/s41586-019-1163-x Bibcode: 2019Natur.569E...1V

Montmessin, Franck; Belyaev, Denis A.; Fedorova, Anna A. +65 more

The surname of author Cathy Quantin-Nataf was misspelled `Quantin-Nata' , authors Ehouarn Millour and Roland Young were missing from the ACS Science Team list, and minor changes have been made to the author and affiliation lists; see accompanying Amendment. These errors have been corrected online.

2019 Nature
ExoMars-16 0
Catalogue of Visual Binaries in Gaia DR2
DOI: 10.26087/INASAN.2019.3.1.057 Bibcode: 2019INASR...3..366S

Kovaleva, D. A.; Sapozhnikov, S. A.; Malkov, O. Y.

We use Gaia DR2 data to construct a catalogue of visual binaries between 10 pc and 100 pc distance from the Sun. Based on data on positions and parallaxes, we have compiled a list of binary candidates containing all pairs of stars positioned within 1 parsec to one another. We have developed an algorithm involving the separation of sky into smaller…

2019 INASAN Science Reports
Gaia 0
Astrometric reduction of Cassini ISS images of Helene
DOI: 10.1360/SSPMA2018-00269 Bibcode: 2019SSPMA..49a9502Z

Peng, Qingyu; Wang, Na; Li, Zhan +3 more

2019 Scientia Sinica Physica, Mechanica & Astronomica
Cassini 0
Investigation of the Effect of a Longitudinal Magnetic Field Component on the Dynamics of Protons inside a Plasmoid
DOI: 10.1134/S0010952519040051 Bibcode: 2019CosRe..57..227M

Malova, H. V.; Malykhin, A. Yu.; Grigorenko, E. E.

Kinetic effects of the dynamics of protons in plasmoids with a non-zero longitudinal ( By) magnetic field component in a current sheet (CS) of a geomagnetic tail are considered. The results of modeling proton dynamics and a description of the mechanism of emergence of "north-south" density asymmetry are presented. The mechanism that is possibly re…

2019 Cosmic Research
Cluster 0
A new sample of southern radio galaxies: host-galaxy masses and star-formation rates
DOI: 10.1093/mnras/stz2371 Bibcode: 2019MNRAS.489.3403M

Jarvis, Matt J.; Prescott, Matthew; Marubini, Takalani +3 more

In this study we define a new sample of distant powerful radio galaxies in order to study their host galaxy properties and provide targets for future observations of H I absorption with new radio telescopes and to understand the fuelling and feedback from such sources. We have cross-matched the Sydney University Molonglo Sky Survey (SUMSS) radio c…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 0
Investigating the OB associations in CMa using eclipsing binary systems: Preliminary results on LV CMa
Bibcode: 2019CoSka..49..430T

Bakış, V.; Tunç, E.

In this study, an eclipsing binary of a short orbital period (P = 1.d1834857) LV CMa (V = 8.m7) is selected as a candidate member of an association in the direction of CMa OB1/R1 region. Light curves in UBVRcIc photometric bands were obtained and low-resolution (R ∼ 5500) spectra were collected. Prelimin…

2019 Contributions of the Astronomical Observatory Skalnate Pleso
Gaia 0
The tricky line of sight towards Cygnus-X: The [DB2001] CL05 embedded cluster as a pilot case
DOI: 10.48550/arXiv.1903.01561 Bibcode: 2019hsax.conf..296D

Jiménez-Bailón, E.; Alves, J.; de la Fuente, D. +2 more

The nearest massive star-forming complex, Cygnus-X, is widely used as a laboratory for star cluster formation and feedback processes, under the implicit assumption that all its components are located roughly at the same distance. We present a multi-wavelength study of a 15' × 15' field in southern Cygnus-X, where different components involving clu…

2019 Highlights on Spanish Astrophysics X
Gaia 0
On the Fon Astroplate Project Accomplishment
DOI: 10.18524/1810-4215.2019.32.181558 Bibcode: 2019OAP....32..185A

Ehgamberdiev, Sh. A.; Andruk, V. M.; Pakuliak, L. K. +10 more

The plan of the photographic survey of the northern sky (FON) was proposed in 1976 in Golosiiv observatory (now MAO NAS of Ukraine) by I. Kolchinsky and A. Onegina. The final project of the Compiled FONAC catalog (FON Astrographic Catalog) is based on the digital data of photographic plates exposed at four observatories. They are MAO NAS of Ukrain…

2019 Odessa Astronomical Publications
Hipparcos 0