Search Publications

Local galaxies with compact cores as the possible descendants of massive compact quiescent galaxies at high redshift
DOI: 10.1088/1674-4527/20/7/106 Bibcode: 2020RAA....20..106G

Fan, Lu-Lu; Gao, Ying

In order to test a possible evolutionary scenario of high-z compact quiescent galaxies (cQGs) that they can survive as local compact cores embedded in local massive galaxies with different morphology classes, we explore the star formation histories of local compact cores according to their spectral analysis. We build a sample of 182 massive galaxi…

2020 Research in Astronomy and Astrophysics
eHST 4
Accuracy of view factor calculations for digital terrain models of comets and asteroids
DOI: 10.1051/0004-6361/202038462 Bibcode: 2020A&A...642A.167R

Rezac, L.; Zhao, Y.

Context. Detailed shape and topographic models coupled with sophisticated thermal physics are critical elements to proper characterization of surfaces of small bodies in our solar system. Calculations of self-heating effects are especially important in the context of thermal evolution of non-convex surfaces, including craters, cracks, or openings …

2020 Astronomy and Astrophysics
Rosetta 4
On the Long Range Clustering of Global Seismicity and its Correlation With Solar Activity: A New Perspective for Earthquake Forecasting
DOI: 10.3389/feart.2020.595209 Bibcode: 2020FrEaS...8..470M

Marchitelli, Vito; Troise, Claudia; Harabaglia, Paolo +2 more

Large earthquakes occurring worldwide have long been recognized to be non Poisson distributed, so involving some large scale correlation mechanism, which could be internal or external to the Earth. We have recently demonstrated this observation can be explained by the correlation of global seismicity with solar activity. We inferred such a clear c…

2020 Frontiers in Earth Science
SOHO 4
Statistical Analysis of Asymmetric Sunspot Decay Observed by Hinode
DOI: 10.1007/s11207-020-01724-x Bibcode: 2020SoPh..295..154I

Imada, Shinsuke; Kato, Shota; Fujiyama, Masashi

We statistically studied the transport of magnetic flux in and around sunspots using a magnetic-element tracking technique to investigate whether sunspot-decay processes are isotropic. Using this method, we detected moving magnetic features (MMFs). The observed radius of an MMFs region was approximately 1.7 times the sunspot radius; furthermore, t…

2020 Solar Physics
Hinode 4
On the flux saturation of SOHO/ERNE proton events
Bibcode: 2020BlgAJ..33...99M

Miteva, Rositsa; Dechev, Momchil; Samwel, Susan W. +1 more

This study lists the main procedures completed on the analysis of solar proton events using data from the SOHO/ERNE high energy detector in the period 1996$-$2017. The highest possible temporal resolution of 1 minute is used here. The proton fluxes from the two analyzed energy channels, at $\sim$25 and $\sim$50 MeV, are compared with the respectiv…

2020 Bulgarian Astronomical Journal
SOHO 4
Bright spectroscopic binaries: I. Orbital parameters of five systems with periods of P < 365 days
DOI: 10.1002/asna.202013741 Bibcode: 2020AN....341..616J

Jack, Dennis; Schröder, Klaus-Peter; Hernández Huerta, Missael Alejandro

In a well‑aimed search based on the recently published Gaia DR2 radial velocity data and performed with the robotic TIGRE telescope, we have discovered 19 bright (mV < 7.66 mag) spectroscopic binary stars. We present the radial velocity curves of five of these stars (HD 20656, HD 27259, HD 98812, HD 150600, HD 193082) with periods of P < 365…

2020 Astronomische Nachrichten
Gaia 4
Identification of young nearby runaway stars based on Gaia data and the lithium test
DOI: 10.1002/asna.202013793 Bibcode: 2020AN....341..908B

Torres, Guillermo; Mugrauer, Markus; Lux, Oliver +6 more

Young nearby runaway stars are suitable to search for their place of origin and possibly associated objects, for example, neutron stars. Tetzlaff et al. (2011) selected young (≤50 Myr) runaway star candidates from Hipparcos, for which they had estimated the ages from the location in the Hertzsprung-Russell diagram and evolutionary models. Here, we…

2020 Astronomische Nachrichten
Gaia Hipparcos 4
X-Ray Observations of the Peculiar Cepheid V473 Lyr Identify A Low-mass Companion
DOI: 10.3847/1538-3881/ab7121 Bibcode: 2020AJ....159..121E

Drake, Jeremy J.; Evans, Nancy Remage; Marengo, Massimo +17 more

V473 Lyr is a classical Cepheid that is unique in having substantial amplitude variations with a period of approximately 3.3 yr, thought to be similar to the Blazhko variations in RR Lyrae stars. We obtained an XMM-Newton observation of this star to follow up a previous detection in X-rays. Rather than the X-ray burst and rapid decline near maximu…

2020 The Astronomical Journal
Gaia XMM-Newton eHST 4
Dust and gas in the central region of NGC 1316 (Fornax A). Its origin and nature
DOI: 10.1051/0004-6361/202038150 Bibcode: 2020A&A...643A.120R

Hilker, M.; Richtler, T.; Iodice, E.

Context. The early-type galaxy NGC 1316, associated with the radio source Fornax A, hosts about 107 M of dust within a central radius of 5 kpc. These prominent dust structures are believed to have an external origin, which is also a popular interpretation for other dusty early-type galaxies. Moreover, it has been long known …

2020 Astronomy and Astrophysics
eHST 4
First speckle interferometric measurements of binary stars at the Observatorio Astrofísico Guillermo Haro
DOI: 10.1093/mnras/staa1236 Bibcode: 2020MNRAS.495..806G

Guerrero, C. A.; Castillo, E.; Rosales-Ortega, F. F. +4 more

In this paper, we present the first multiband speckle interferometric measurements of binary stars performed using the 2.1 m telescope of the Observatorio Astrofísico Guillermo Haro, Cananea, Sonora, México. We describe here FICCO: Fast Imaging Camera for Cananea Observatory, a new instrument developed to perform speckle observations from the Nort…

2020 Monthly Notices of the Royal Astronomical Society
Hipparcos 4