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pro vyhledávání: '"Neelam Panwar"'
The processes which regulate the star-formation within molecular clouds are still not well understood. Various star-formation scaling relations have been proposed to explain this issue by formulating a relation between star-formation rate surface den
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e95caa3746bf28cd067d9269968b216b
http://arxiv.org/abs/2010.07333
http://arxiv.org/abs/2010.07333
Autor:
Rakesh Pandey, Lokesh K. Dewangan, Devendra K. Ojha, Tirthendu Sinha, Anil K. Pandey, D. P. Bisen, Arpan Ghosh, Saurabh Sharma, Neelam Panwar
Using our deep optical and near-infrared photometry along with multiwavelength archival data, we here present a detailed study of the Galactic H II region Sh 2-305, to understand the star/star-cluster formation. On the basis of excess infra-red emiss
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::029de46b68a1dcff1b8c4be731f69a5c
http://arxiv.org/abs/2001.04722
http://arxiv.org/abs/2001.04722
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, Jessy Jose, Manash R. Samal, Katsuo Ogura, Wen Ping Chen, Harinder P. Singh, R. K. Yadav, D. K. Ojha, Ashwani Pandey
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2017, 468 (3), pp.2684-2698. ⟨10.1093/mnras/stx616⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2017, 468 (3), pp.2684-2698. ⟨10.1093/mnras/stx616⟩
Monthly Notices of the Royal Astronomical Society, 2017, 468 (3), pp.2684-2698. ⟨10.1093/mnras/stx616⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2017, 468 (3), pp.2684-2698. ⟨10.1093/mnras/stx616⟩
W4 is a giant H{\sc ii} region ionized by the OB stars of the cluster IC~1805. The H{\sc ii} region/cluster complex has been a subject of numerous investigations as it is an excellent laboratory for studying the feedback effect of massive stars on th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1f16344b594aea5400f823e74902a4ad
http://arxiv.org/abs/1703.03604
http://arxiv.org/abs/1703.03604
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