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pro vyhledávání: '"Neelam Panwar"'
It is well known that most of the stars form in rich clusters. However, recent $Spitzer$ observations have shown that a significant number of stars also form in distributed mode, origin of which is not well understood. In this work, we aim to investi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7b9a4c67a8d40538b344eaba6a456858
http://arxiv.org/abs/1901.00888
http://arxiv.org/abs/1901.00888
Autor:
Neelam Panwar, Wen Ping Chen, Paolo Battinelli, Katsuo Ogura, Manash R. Samal, Ashwani Pandey, Harinder P. Singh, Devendra K. Ojha
Berkeley 59 is a nearby ($\sim$1 kpc) young cluster associated with the Sh2-171 H{\sc ii} region. We present deep optical observations of the central $\sim$2.5$\times$2.5 pc$^2$ area of the cluster, obtained with the 3.58-m Telescopio Nazionale Galil
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b79f8d87c900a298b4f996a21dbc5490
http://arxiv.org/abs/1711.09353
http://arxiv.org/abs/1711.09353
The evolution of HII regions/supershells can trigger a new generation of stars/clusters at their peripheries, with environmental conditions that may affect the initial mass function, disk evolution and star formation efficiency. In this paper we stud
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9d3e04d727c8b1e7b8bcb0f1b68f0505