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Analyzing the dynamical state of nearby young massive star clusters is essential understanding star cluster formation and evolution during their earliest stages. In this work we analyze the stellar and gas kinematics of the young massive…

Solar and Stellar Astrophysics · Physics 2021-03-03 Peter Zeidler , Elena Sabbi , Antonella Nota , Anna F. McLeod

Westerlund 2 (Wd2) is the central ionizing star cluster of the \ion{H}{2} region RCW~49 and the second most massive young star cluster (${\rm M} = (3.6 \pm 0.3)\times 10^4\,{\rm M}_\odot$) in the Milky Way. Its young age ($\sim2\,$Myr) and…

An unsettled question concerning the formation and distribution of massive stars is whether they must be born in massive clusters and, if found in less dense environments, whether they must have migrated there. With the advent of wide-area…

Solar and Stellar Astrophysics · Physics 2018-08-01 J. E. Drew , A. Herrero , M. Mohr-Smith , M. Monguio , N. J. Wright , T. Kupfer , R. Napiwotzki

We present a spectroscopic and photometric determination of the distance to the young Galactic open cluster Westerlund 2 using WFPC2 imaging from the Hubble Space Telescope and ground-based optical spectroscopy. HST imaging in the F336W,…

The Galactic open cluster Westerlund 1 (Wd 1) represents the ideal local template for extragalactic young massive star clusters, because it is currently the only nearby young cluster which reaches a mass of around 10^5 Msun. The proximity…

Astrophysics · Physics 2009-12-04 S. Mengel , L. E. Tacconi-Garman

The Galactic open cluster Westerlund 1 was found only a few years ago to be much more massive than previously thought, with evidence suggesting its mass to be in excess of ~10^5 Msun, in the range spanned by young extragalactic star…

Astrophysics · Physics 2009-11-13 Sabine Mengel , Lowell E. Tacconi-Garman

We present a structural analysis of the young massive star cluster Westerlund 1 (Wd 1). With multi-epoch Hubble Space Telescope (HST) observations, we measure the proper motions of $10346$ stars and determine their kinematic memberships by…

Time-domain studies of pre-main sequence stars have long been used to investigate star properties during their early evolutionary phases and to trace the evolution of circumstellar environments. Historically these studies have been confined…

Solar and Stellar Astrophysics · Physics 2020-03-25 E. Sabbi , M. Gennaro , J. Anderson , V. Bajaj , N. Bastian , J. S. Gallagher , III , M. Gieles , D. J. Lennon , A. Nota , K. C. Sahu , P. Zeidler

Being the most massive known young stellar cluster in the Milky Way, Westerlund 1 (Wd1) constitutes an ideal benchmark for understanding the evolution of massive stars. However, the cluster age remains highly controversial (~4-10 Myr),…

We present the results of current observations of the young compact cluster of massive stars Westerlund 2 with the Mikhail Pavlinsky ART-XC telescope aboard the Spectrum-Roentgen-Gamma (SRG) observatory which we analysed together with the…

High Energy Astrophysical Phenomena · Physics 2023-09-11 A. M. Bykov , Yu. A. Uvarov , M. E. Kalyashova , D. V. Badmaev , I. Yu. Lapshov , A. A. Lutovinov , I. A. Mereminskiy , A. N. Semena

Massive stellar clusters are the best available laboratories to study the mass function of stars. Based on NTT/SofI near-infrared photometry, we have investigated the properties of the massive young cluster Westerlund 1. From comparison…

Astrophysics of Galaxies · Physics 2015-05-20 Mario Gennaro , Wolfgang Brandner , Andrea Stolte , Thomas Henning

Young massive stellar clusters are extreme environments and potentially provide the means for efficient particle acceleration. Indeed, they are increasingly considered as being responsible for a significant fraction of cosmic rays (CRs)…

High Energy Astrophysical Phenomena · Physics 2022-11-11 F. Aharonian , H. Ashkar , M. Backes , V. Barbosa Martins , Y. Becherini , D. Berge , B. Bi , M. Böttcher , M. de Bony de Lavergne , F. Bradascio , R. Brose , F. Brun , T. Bulik , C. Burger-Scheidlin , F. Cangemi , S. Caroff , S. Casanova , M. Cerruti , T. Chand , S. Chandra , A. Chen , O. Chibueze , P. Cristofari , J. Damascene Mbarubucyeye , A. Djannati-Ataï , J. -P. Ernenwein , K. Feijen , G. Fichet de Clairfontaine , G. Fontaine , S. Funk , S. Gabici , Y. A. Gallant , S. Ghafourizadeh , G. Giavitto , L. Giunti , D. Glawion , J. F. Glicenstein , P. Goswami , M. -H. Grondin , L. K. Härer , M. Haupt , J. A. Hinton , M. Hörbe , W. Hofmann , T. L. Holch , M. Holler , D. Horns , M. Jamrozy , V. Joshi , I. Jung-Richardt , E. Kasai , K. Katarzyński , U. Katz , B. Khélifi , W. Kluźniak , Nu. Komin , K. Kosack , D. Kostunin , G. Kukec Mezek , R. G. Lang , S. Le Stum , A. Lemière , M. Lemoine-Goumard , J. -P. Lenain , F. Leuschner , T. Lohse , A. Luashvili , I. Lypova , J. Mackey , J. Majumdar , D. Malyshev , V. Marandon , P. Marchegiani , A. Marcowith , G. Martí-Devesa , R. Marx , G. Maurin , M. Meyer , A. Mitchell , R. Moderski , L. Mohrmann , A. Montanari , E. Moulin , J. Muller , T. Murach , K. Nakashima , M. de Naurois , A. Nayerhoda , J. Niemiec , S. Ohm , L. Olivera-Nieto , E. de Ona Wilhelmi , M. Ostrowski , S. Panny , M. Panter , R. D. Parsons , G. Peron , D. A. Prokhorov , G. Pühlhofer , M. Punch , A. Quirrenbach , R. Rauth , P. Reichherzer , A. Reimer , O. Reimer , M. Renaud , B. Reville , F. Rieger , G. Rowell , B. Rudak , E. Ruiz-Velasco , V. Sahakian , H. Salzmann , D. A. Sanchez , A. Santangelo , M. Sasaki , F. Schüssler , H. M. Schutte , U. Schwanke , J. N. S. Shapopi , A. Specovius , S. Spencer , Ł. Stawarz , R. Steenkamp , S. Steinmassl , C. Steppa , I. Sushch , H. Suzuki , T. Takahashi , T. Tanaka , R. Terrier , C. Thorpe-Morgan , M. Tsirou , N. Tsuji , R. Tuffs , T. Unbehaun , C. van Eldik , B. van Soelen , M. Vecchi , J. Veh , C. Venter , J. Vink , S. J. Wagner , R. White , A. Wierzcholska , Yu Wun Wong , M. Zacharias , D. Zargaryan , A. A. Zdziarski , S. J. Zhu , S. Zouari , N. Żywucka , R. Blackwell , C. Braiding , M. Burton , K. Cubuk , M. Filipović , N. Tothill , G. Wong

We present a detailed analysis of the pre-main-sequence (PMS) population of the young star cluster Westerlund~2 (Wd2), the central ionizing cluster of the HII region RCW 49, using data from a high resolution multi-band survey with the…

Solar and Stellar Astrophysics · Physics 2016-09-19 Peter Zeidler , Eva K. Grebel , Antonella Nota , Elena Sabbi , Anna Pasquali , Monica Tosi , Alceste Z. Bonanos , Carol Christian

We present a time-variability study of young stellar objects in the cluster IRAS 20050+2720, performed at 3.6 and 4.5 micron with the Spitzer Space Telescope; this study is part of the Young Stellar Object VARiability project (YSOVAR). We…

Detailed studies of resolved young massive star clusters are necessary to determine their dynamical state and evaluate the importance of gas expulsion and early cluster evolution. In an effort to gain insight into the dynamical state of the…

O-type stars are known to significantly contribute to both the dynamics and evolution of galaxies. Massive and luminous, they probably control and regulate the galaxies star formation rates. For this work I performed a redetermination of…

Solar and Stellar Astrophysics · Physics 2024-04-26 A. Roman-Lopes

We present a detailed analysis of the spatial distribution of the stellar population and the present-day mass function (PDMF) of the Westerlund 2 (Wd2) region using the data from our high resolution multi-band survey with the Hubble Space…

Astrophysics of Galaxies · Physics 2017-02-24 Peter Zeidler , Antonella Nota , Eva K. Grebel , Elena Sabbi , Anna Pasquali , Monica Tosi , Carol Christian

We present first results from a high resolution multi-band survey of the Westerlund 2 region with the Hubble Space Telescope. Specifically, we imaged Westerlund 2 with the Advanced Camera for Surveys through the $F555W$, $F814W$, and…

Aims. The properties of the early-type stars in the core of the Westerlund2 cluster are examined in order to establish a link between the cluster and the very massive Wolf-Rayet binary WR20a as well as the HII complex RCW49. Methods.…

Astrophysics · Physics 2020-12-09 G. Rauw , J. Manfroid , E. Gosset , Y. Naze , H. Sana , M. De Becker , C. Foellmi , A. F. J. Moffat

We present 5201 radial-velocity measurements of 1144 stars, as part of an ongoing study of the young (150 Myr) open cluster M35 (NGC 2168). We have observed M35 since 1997, using the Hydra Multi-Object Spectrograph on the WIYN 3.5m…

Solar and Stellar Astrophysics · Physics 2015-05-14 Aaron M. Geller , Robert D. Mathieu , Ella K. Braden , Soren Meibom , Imants Platais , Christopher J. Dolan
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