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19922026
most citedThe Sloan Digital Sky Survey: Technical Summary

10.4k citations

Showing 2017 · astro-ph.SRShow all

28 papers · 2 filters

astro-ph.SR2017★ 8 cited

An application of the weighted horizontal magnetic gradient to solar compact and eruptive events

M. B. Korsos, Michael S. Ruderman, R. Erdelyi

We propose to apply the weighted horizontal magnetic gradient (), introduced in Korsos et al (2015), for analysing the pre-flare and pre-CME behaviour and evolution of Acti…

astro-ph.SR2017★ 29 cited

A new compact young moving group around V1062 Sco

Siegfried Röser, Elena Schilbach, Bertrand Goldman +3

Aims. We are searching for new open clusters or moving groups in the Solar neighbourhood. Methods. We used the Gaia-TGAS catalogue, cut it into narrow proper motion and parallax sl…

astro-ph.SR2017★ 6 cited

A Photometric Study of Globular Clusters Observed by the APOGEE Survey

Szabolcs Mészáros, D. A. García-Hernández, Santi Cassisi +8

In this paper we describe the photometric and spectroscopic properties of multiple populations in seven northern globular clusters. In this study we employ precise ground based pho…

astro-ph.SR2017★ 25 cited

An UXor among FUors: extinction related brightness variations of the young eruptive star V582 Aur

P. Ábrahám, Á. Kóspál, M. Kun +24

V582 Aur is an FU Ori-type young eruptive star in outburst since 1985. The eruption is currently in a relatively constant plateau phase, with photometric and spectroscopic va…

astro-ph.SR2017★ 32 cited

A view of the H-band light-element chemical patterns in Globular Clusters under the AGB self-enrichment scenario

F. Dell'Agli, D. A. García-Hernández, P. Ventura +7

We discuss the self-enrichment scenario by AGB stars for the formation of multiple populations in globular clusters (GCs) by analyzing data set of giant stars observed in 9 Galacti…

astro-ph.SR2017★ 90 cited

The Effect of "Rogue" Active Regions on the Solar Cycle

Melinda Nagy, Alexandre Lemerle, François Labonville +2

The origin of cycle-to-cycle variations in solar activity is currently the focus of much interest. It has recently been pointed out that large individual active regions with atypic…

astro-ph.SR2017★ 24 cited

12C/13C isotopic ratios in red-giant stars of the open cluster NGC 6791

László Szigeti, Szabolcs Mészáros, Verne V. Smith +10

Carbon isotope ratios, along with carbon and nitrogen abundances, are derived in a sample of 11 red-giant members of one of the most metal-rich clusters in the Milky Way, NGC 6791.…

astro-ph.SR2017★ 7 cited

Dissipative instabilities in a partially ionised prominence plasma slab: II. The effect of compressibility

J. F. Mather, I. Ballai, R. Erdelyi

This present study deals with the dissipative instability that appears in a compressible partially ionised plasma slab embedded in a uniform magnetic field, modelling the state of…

astro-ph.SR2017★ 15 cited

Observations of Running Penumbral Waves emerging in a Sunspot

T. G. Priya, Wenda Cao, Jiangtao Su +4

We present results from the investigation of 5-min umbral oscillations in a single-polarity sunspot of active region NOAA 12132. The spectra of TiO, H, and 304 Å are used for co…

astro-ph.SR2017★ 14 cited

Untwisting Jets Related to Magnetic Flux Cancellation

Jiajia Liu, Robert Erdélyi, Yuming Wang +1

The rotational motion of solar jets is believed to be a signature of the untwisting process resulting from magnetic reconnection, which takes place between twisted closed magnetic…

astro-ph.SR2017

Predicting the Loci of Solar Eruptions

N. Gyenge, R. Erdélyi

The longitudinal distribution of solar active regions shows non-homogeneous spatial behaviour, which is often referred to as Active Longitude (AL). Evidence for a significant stati…

astro-ph.SR2017★ 25 cited

Rotation--differential rotation relationships for late-type single and binary stars from Doppler imaging

Zs. Kővári, K. Oláh, L. Kriskovics +3

From our sample of spotted late-type stars showing surface differential rotation we find that the relationship between the rotation period and the surface shear coefficient $α=ΔΩ/Ω…

astro-ph.SR2017★ 23 cited

Interferometric view of the circumstellar envelopes of northern FU Orionis-type stars

O. Fehér, Á. Kóspál, P. Ábrahám +2

FU Orionis-type objects are young, low-mass stars with large outbursts in visible light that last for several years or decades. They are thought to represent an evolutionary phase…

astro-ph.SR2017★ 34 cited

The Frequency-dependent Damping of Slow Magnetoacoustic Waves in a Sunspot Umbral Atmosphere

S. Krishna Prasad, D. B. Jess, T. Van Doorsselaere +5

High spatial and temporal resolution images of a sunspot, obtained simultaneously in multiple optical and UV wavelengths, are employed to study the propagation and damping characte…

astro-ph.SR2017★ 16 cited

Antisolar differential rotation with surface lithium enrichment on the single K-giant V1192 Orionis

Zs. Kővári, K. G. Strassmeier, T. A. Carroll +7

Context: Stars with about 12 solar masses at the red giant branch (RGB) represent an intriguing period of stellar evolution, i.e. when the convective envelope interacts with the…

astro-ph.SR2017★ 10 cited

Large amplitude change in spot-induced rotational modulation of the Kepler Ap star KIC 2569073

Jason A. Drury, Simon J. Murphy, Aliz Derekas +9

An investigation of the 200 200 pixel 'superstamp' images of the centres of the open clusters NGC 6791 and NGC 6819 allows for the identification and study of many variabl…

astro-ph.SR2017★ 47 cited

IRIS Burst Spectra Co-Spatial To A Quiet-Sun Ellerman-Like Brightening

C. J. Nelson, N. Freij, A. Reid +3

Ellerman bombs (EBs) have been widely studied over the past two decades; however, only recently have counterparts of these events been observed in the quiet-Sun. The aim of this ar…

astro-ph.SR2017★ 12 cited

Sunspot Light Walls Suppressed by Nearby Brightenings

Shuhong Yang, Jun Zhang, Robertus Erdélyi +3

Light walls, as ensembles of oscillating bright structures rooted in sunspot light bridges, have not been well studied, although they are important for understanding sunspot proper…

astro-ph.SR2017★ 25 cited

A search for tight hierarchical triple systems amongst the eclipsing binaries in the CoRoT fields

T. Hajdu, T. Borkovits, E. Forgács-Dajka +5

We report a comprehensive search for hierarchical triple stellar system candidates amongst eclipsing binaries (EB) observed by the CoRoT spacecraft. We calculate and check eclipse…

astro-ph.SR2017

The MOST view of Cepheids

L. Molnár, A. Derekas, R. Szabó +6

The MOST space telescope observed four Cepheid variables so far, all of different subtypes. Here we summarize the results obtained and the possible ways to continue to study these…

astro-ph.SR2017★ 174 cited

Frequent flaring in the TRAPPIST-1 system - unsuited for life?

Krisztián Vida, Zsolt Kővári, András Pál +2

We analyze short cadence K2 light curve of the TRAPPIST-1 system. Fourier analysis of the data suggests days. The light curve shows several flares, o…

astro-ph.SR2017★ 129 cited

The Correlation Between Mixing Length and Metallicity on the Giant Branch: Implications for Ages in the Gaia Era

Jamie Tayar, Garrett Somers, Marc H. Pinsonneault +28

In the updated APOGEE-Kepler catalog, we have asteroseismic and spectroscopic data for over 3000 first ascent red giants. Given the size and accuracy of this sample, these data off…

astro-ph.SR2017★ 147 cited

A New Stellar Atmosphere Grid and Comparisons with HST/STIS Calspec Flux Distributions

Ralph C. Bohlin, Szabolcs Meszaros, Scott W. Fleming +3

The Space Telescope Imaging Spectrograph (STIS) has measured the spectral energy distributions (SEDs) for several stars of types O, B, A, F, and G. These absolute fluxes from the C…

astro-ph.SR2017★ 61 cited

MARVEL analysis of the measured high-resolution rovibronic spectra of TiO

Laura K. McKemmish, Thomas Masseron, Samuel Sheppard +6

Accurate, experimental rovibronic energy levels, with associated labels and uncertainties, are reported for 11 low-lying electronic states of the diatomic \TiO\ molecule, determine…