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20132026
most citedThe KELT Follow-Up Network and Transit False Positive Catalog: Pre-vetted False Positives for TESS

77 citations · 261 across the 26 of their papers we have counts for

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17 papers · 1 filter

astro-ph.SR2026

A survey for variable young stars with small telescopes - XI. Spot Lifetimes and Coverage Distributions

Dirk Froebrich, Carys Herbert, Aleks Scholz +47

We present a homogeneous analysis of rotational variability and spot properties in young stellar objects across multiple star-forming regions observed by the Hunting Outbursting Yo…

astro-ph.SR2025

Is the Symbiotic Recurrent Nova T CrB Late? Recent Photometric Evolution and Comparison with Past Pre-Outburst Behaviour

Jaroslav Merc, Łukasz Wyrzykowski, Paul G. Beck +46

T CrB is a symbiotic recurrent nova that last erupted in 1946. Given its recurrence timescale of approximately 80 years, the next outburst is eagerly anticipated by the astronomica…

astro-ph.SR2024

A survey for variable stars with small telescopes: IX -- Evolution of Spot Properties on YSOs in IC5070

Carys Herbert, Dirk Froebrich, Siegfried Vanaverbeke +45

We present spot properties on 32 periodic young stellar objects in IC 5070. Long term, 5 yr, light curves in the , , and -bands are obtained through the HOYS (Huntin…

astro-ph.SR2024

A survey for variable young stars with small telescopes: VIII -- Properties of 1687 Gaia selected members in 21 nearby clusters

Dirk Froebrich, Aleks Scholz, Justyn Campbell-White +60

The Hunting Outbursting Young Stars (HOYS) project performs long-term, optical, multi-filter, high cadence monitoring of 25 nearby young clusters and star forming regions. Utilisin…

astro-ph.SR2024

CARMENES input catalog of M dwarfs: VII. New rotation periods for the survey stars and their correlations with stellar activity

Yutong Shan, Daniel Revilla, Sebastian L. Skrzypinski +40

Abridged: We measured photometric and spectroscopic for a large sample of nearby bright M dwarfs with spectral types from M0 to M9, as part of our continual effort to…

astro-ph.SR2023

TESS photometry of the nova eruption in V606 Vul: asymmetric photosphere and multiple ejections?

Kirill V. Sokolovsky, Elias Aydi, Konstantin Malanchev +70

Lightcurves of many classical novae deviate from the canonical "fast rise - smooth decline" pattern and display complex variability behavior. We present the first TESS-space-photom…

astro-ph.SR2023★ 5 cited

A survey for variable young stars with small telescopes: VI -- Analysis of the outbursting Be stars NSW284, Gaia19eyy, and VES263

Dirk Froebrich, Lynne A. Hillenbrand, Carys Herbert +44

This paper is one in a series reporting results from small telescope observations of variable young stars. Here, we study the repeating outbursts of three likely Be stars based on…

astro-ph.SR2022★ 4 cited

Variability of eclipse timing:the case of V471 Tauri

Emil Kundra, Ľubomír Hambálek, Siegfried Vanaverbeke +4

The post-common envelope binary V471 Tauri has been an object of interest for decades. V471 Tau shows various phenomena due to its evolutionary state and unique properties, e.g. it…

astro-ph.SR2021★ 5 cited

Turbulence and its connection to episodic accretion in binary YSOs

Rafeel Riaz, Dominik R. G. Schleicher, Siegfried Vanaverbeke +1

We report signatures of episodic accretion in young stellar objects (YSOs) that emerge in protobinary configurations in a gravoturbulent gas collapse. We find in most of these prot…

astro-ph.SR2021★ 9 cited

A survey for variable young stars with small telescopes: IV -- Rotation Periods of YSOs in IC5070

Dirk Froebrich, Efthymia Derezea, Aleks Scholz +50

Studying rotational variability of young stars is enabling us to investigate a multitude of properties of young star-disk systems. We utilise high cadence, multi-wavelength optical…

astro-ph.SR2020★ 7 cited

An Asymmetric Eclipse Seen Towards the Pre-Main Sequence Binary System V928 Tau

Dirk van Dam, Matthew Kenworthy, Trevor David +21

K2 observations of the weak-lined T Tauri binary V928 Tau A+B show the detection of a single, asymmetric eclipse which may be due to a previously unknown substellar companion eclip…

astro-ph.SR2018★ 12 cited

The KIC 8462852 Light Curve From 2015.75 to 2018.18 Shows a Variable Secular Decline

Bradley E. Schaefer, Rory O. Bentley, Tabetha S. Boyajian +19

The star KIC 8462852 (Boyajian's Star) displays both fast dips of up to 20% on time scales of days, plus long-term secular fading by up to 19% on time scales from a year to a centu…

astro-ph.SR2018★ 12 cited

Formation of multiple low mass stars, brown dwarfs and planemos via gravitational collapse

Rafeel Riaz, Siegfried Vanaverbeke, Dominik R. G. Schleicher

The origin of very low-mass stars (VLMS) and brown dwarfs (BDs) is still an unresolved topic of star formation. We here present numerical simulations of the formation of VLMS, BDs,…

astro-ph.SR2017★ 5 cited

Episodic accretion in binary protostars emerging from self-gravitating solar mass cores

R. Riaz, S. Vanaverbeke, D. R. G. Schleicher

Observations show a large spread in the luminosities of young protostars, which are frequently explained in the context of episodic accretion. We here test this scenario using nume…

astro-ph.SR2016★ 10 cited

RZ Leonis Minoris Bridging between ER Ursae Majoris-Type Dwarf Nova and Novalike System

Taichi Kato, Ryoko Ishioka, Keisuke Isogai +64

We observed RZ LMi, which is renowned for the extremely (~19d) short supercycle and is a member of a small, unusual class of cataclysmic variables called ER UMa-type dwarf novae, i…

astro-ph.SR2016★ 5 cited

NSV 1907 - A new eclipsing, nova-like cataclysmic variable

Stefan Hümmerich, Rainer Gröbel, Franz-Josef Hambsch +6

NSV 1907, formerly listed as an irregular variable in variability catalogues, was classified as an Algol-type eclipsing binary in the Catalina Surveys Periodic Variable Star Catalo…

astro-ph.SR2013★ 1 cited

The early phase of multiple proto-stellar system emerged from collapse of molecular cloud under various initial thermal states

Rafil Riaz, Suhail Zaki Farooqui, Siegfried Vanaverbeke

An attempt is made here to revisit structure formation in a proto-stellar cloud during the early phase of evolution. Molecular cloud subjected to a set of various initial condition…