A Zwicky Transient Facility Look at Optical Variability of Young Stellar Objects in the North America and Pelican Nebulae Complex
LA Hillenbrand, TJ Kiker, M Gee, O Lester… - The Astronomical …, 2022 - iopscience.iop.org
We present a study of 323 photometrically variable young stellar objects that are likely
members of the North America and Pelican nebulae star-forming region. To do so, we utilize …
members of the North America and Pelican nebulae star-forming region. To do so, we utilize …
Gaia 19ajj: A Young Star Brightening Due to Enhanced Accretion and Reduced Extinction
LA Hillenbrand, B Reipurth, M Connelley… - The Astronomical …, 2019 - iopscience.iop.org
We report on the source Gaia 19ajj, identifying it as a young star associated with a little-
studied star-forming region seen along a complex line of sight through the Gum Nebula. The …
studied star-forming region seen along a complex line of sight through the Gum Nebula. The …
Long-term variability of T Tauri stars using WASP
L Rigon, A Scholz, D Anderson… - Monthly Notices of the …, 2017 - academic.oup.com
We present a reference study of the long-term optical variability of young stars using data
from the WASP project. Our primary sample is a group of well-studied classical T Tauri stars …
from the WASP project. Our primary sample is a group of well-studied classical T Tauri stars …
Long-term Photometric Study of the Pre-main Sequence Star V1180 Cas
In this paper results from the optical photometric observations of the pre-main sequence star
V1180 Cas are reported. The star is a young variable associated with the dark cloud Lynds …
V1180 Cas are reported. The star is a young variable associated with the dark cloud Lynds …
T Tauri stars in the SuperWASP and NSVS surveys
Ľ Hambálek, M Vaňko, E Paunzen… - Monthly Notices of the …, 2019 - academic.oup.com
We present a study of the long-term optical variability of young T Tauri stars using previously
unpublished data from the Super-Wide Angle Search for Planets (SuperWASP) project …
unpublished data from the Super-Wide Angle Search for Planets (SuperWASP) project …
Study of the Long-term BVR c I c Photometric Variability of Eight PMS Stars in the Young Open Cluster Trumpler 37
S Ibryamov, G Zidarova, E Semkov… - Research in Astronomy …, 2023 - iopscience.iop.org
This paper reports results from our long-term BV (RI) c photometric CCD observations of
eight pre-main sequence stars collected from 2008 June to 2022 October. These stars are …
eight pre-main sequence stars collected from 2008 June to 2022 October. These stars are …
The pre-main-sequence star V1184 Tauri (CB 34V) at the end of prolonged eclipse
Aims. V1184 Tau (CB 34V) lies in the field of the Bok globule CB 34 and was discovered as
a large amplitude variable in 1993. According to the first hypothesis of the variability of the …
a large amplitude variable in 1993. According to the first hypothesis of the variability of the …
Pre-main sequence stars
E Semkov - arXiv preprint arXiv:2307.01659, 2023 - arxiv.org
The dissertation presents result from study of Pre-main sequence (PMS) stars that are in the
earliest stages of stellar evolution. These young stellar objects are still in the process of …
earliest stages of stellar evolution. These young stellar objects are still in the process of …
V2492 Cygni: Optical BVRI Variability During the Period 2010–2017
Results from BVRI photometric observations of the young stellar object V2492 Cyg collected
during the period from August 2010 to December 2017 are presented. The star is located in …
during the period from August 2010 to December 2017 are presented. The star is located in …
Long-time photometric study of UX Orionis stars
Results from long-term optical photometric observations of the pre-main sequence stars from
UX Orionis type are reported. The UBVRI CCD observations were performed in two …
UX Orionis type are reported. The UBVRI CCD observations were performed in two …