activity
20172024
most citedGaia 18dvy: a new FUor in the Cygnus OB3 association

48 citations · 127 across the 17 of their papers we have counts for

collaborators

18 papers

astro-ph.EP2024

Search for Stellar Companions of Exoplanet Host Stars with AstraLux/CAHA 2.2 m

S. Schlagenhauf, M. Mugrauer, C. Ginski +3

Stellar multiplicity is a key aspect of exoplanet diversity, as the presence of more than one star in a planetary system can have both devastating and positive effects on its forma…

astro-ph.SR2023

The deep eclipses of RW Aur revisited by long-term photometric and spectroscopic monitoring

O. Lux, M. Mugrauer, R. Bischoff

RW Aurigae is a young stellar system containing a classical T Tauri star as the primary component. It shows deep, irregular dimmings, first detected in 2010. At the University Obse…

astro-ph.EP2023

Search for planets in hot Jupiter systems with multi-sector TESS photometry. III. A study of ten systems enhanced with new ground-based photometry

G. Maciejewski, M. Fernández, A. Sota +12

The loneliness of hot Jupiters supports the high-eccentricity migration as a primary path leading to the formation of systems with those planets stripped of any close-in planetary…

astro-ph.EP2022★ 11 cited

Planet-star interactions with precise transit timing. III. Entering the regime of dynamical tides

G. Maciejewski, M. Fernandez, A. Sota +14

Hot Jupiters on extremely short-period orbits are expected to be unstable to tidal dissipation and spiral toward their host stars. That is because they transfer the angular momentu…

astro-ph.EP2022★ 2 cited

YETI follow-up observations of the T Tauri star CVSO30 with transit-like dips

R. Bischoff, St. Raetz, M. Fernández +13

The T Tauri star CVSO30, also known as PTFO8-8695, was studied intensively with ground based telescopes as well as with satellites over the last decade. It showed a variable light…

astro-ph.SR2022★ 12 cited

The origin of the high-mass X-ray binary 4U 2206+54/BD +53 2790

V. Hambaryan, K. A. Stoyanov, M. Mugrauer +7

Based on the Gaia EDR3 astrometric parameters and our new systemic radial velocity of the high-mass X-ray binary 4U 2206+54/BD+53 2790, we studied the trace back motion of the syst…

astro-ph.SR2021

Identification of additional young nearby runaway stars based on Gaia data release 2 observations and the lithium test

R. Bischoff, M. Mugrauer, G. Torres +4

Runaway stars are characterised by their remarkably high space velocities, and the study of their formation mechanisms has attracted considerable interest. Young, nearby runaway st…

astro-ph.EP2021★ 3 cited

Follow-up spectroscopy of comet C/2020 F3 (NEOWISE)

Richard Bischoff, Markus Mugrauer

We present spectroscopy of the coma center of comet C/2020 F3 (NEOWISE), carried out at the end of July 2020 with the Échelle spectrograph FLECHAS at the University Observatory Jen…

astro-ph.SR2021★ 13 cited

A search for runaway stars in twelve Galactic supernova remnants

O. Lux, R. Neuhäuser, M. Mugrauer +1

Runaway stars can result from core-collapse supernovae in multiple stellar systems. If the supernova disrupts the system, the companion gets ejected with its former orbital velocit…

astro-ph.SR2020★ 2 cited

Spectroscopic orbit determination of the long-periodic binary system Cep

R. Bischoff, M. Mugrauer, O. Lux +4

In 2015 a radial velocity monitoring campaign was started in order to redetermine and/or constrain the orbital solutions of spectroscopic binary systems. The observations were carr…

astro-ph.SR2020★ 4 cited

Identification of young nearby runaway stars based on Gaia data and the lithium test

R. Bischoff, M. Mugrauer, G. Torres +6

Young nearby runaway stars are suitable to search for their place of origin and possibly associated objects, for example neutron stars. Tetzlaff, Neuhäuser & Hohle (2011) selected…

astro-ph.SR2020★ 48 cited

Gaia 18dvy: a new FUor in the Cygnus OB3 association

E. Szegedi-Elek, P. Ábrahám, L. Wyrzykowski +59

We present optical-infrared photometric and spectroscopic observations of Gaia18dvy, located in the Cygnus OB3 association at a distance of 1.88 kpc. The object was noted by the Ga…

astro-ph.EP2020

Follow-up imaging observations of comet 2I/Borisov

M. Mugrauer, R. Bischoff, W. Stenglein +3

Follow-up imaging observations of the first detected interstellar comet 2I/Borisov are presented, which were carried out with the Schmidt-Teleskop-Kamera at the University Observat…

astro-ph.SR2019★ 4 cited

Spectroscopic characterization of nine binary star systems as well as HIP107136 and HIP107533

T. Heyne, M. Mugrauer, R. Bischoff +6

We present the results of our 2nd radial velocity monitoring campaign, carried out with the Échelle spectrograph FLECHAS at the University Observatory Jena in the course of the Gro…

astro-ph.SR2019★ 8 cited

Diagnosing the Clumpy Protoplanetary Disk of the UXor Type Young Star GM Cephei

P. C. Huang, W. P. Chen, M. Mugrauer +29

UX Orionis stars (UXors) are Herbig Ae/Be or T Tauri stars exhibiting sporadic occultation of stellar light by circumstellar dust. GM\,Cephei is such a UXor in the young (~M…

astro-ph.EP2018

Planet-star interactions with precise transit timing. I. The refined orbital decay rate for WASP-12 b and initial constraints for HAT-P-23 b, KELT-1 b, KELT-16 b, WASP-33 b, and WASP-103 b

G. Maciejewski, M. Fernández, F. Aceituno +11

Theoretical calculations and some indirect observations show that massive exoplanets on tight orbits must decay due to tidal dissipation within their host stars. This orbital evolu…

astro-ph.SR2018★ 7 cited

The Radial and Rotational Velocity of Ophiuchi

T. Zehe, M. Mugrauer, R. Neuhäuser +5

We present the results of our spectroscopic monitoring campaign of Oph, carried out at the University observatory Jena with the spectrograph FLECHAS between July 2015 and Septe…

astro-ph.SR2017★ 13 cited

Radial velocity measurements and orbit determination of eight single-lined spectroscopic binary systems

R. Bischoff, M. Mugrauer, T. Zehe +7

Since early 2015 a new radial velocity monitoring campaign is going on at the University Observatory Jena. The aim of this project is to obtain current radial velocity measurements…