Zobrazeno 1 - 5
of 5
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
Autor:
Neelam Panwar, M. J. Arévalo, Clemens Thum, Antoniya Valcheva, Mark Gurwell, Elena G. Larionova, R. D. Schwartz, S. N. Molina, Evgeni Ovcharov, M. Pasanen, J. Leon-Tavares, J. A. Ros, A. Di Paola, L. V. Larionova, Svetlana G. Jorstad, H. C. Lin, K. Blumenthal, A. Sillanpää, Tatiana S. Konstantinova, D. O. Mirzaqulov, D. A. Morozova, R. Reinthal, Jochen Heidt, Carolina Casadio, Anne Lähteenmäki, Ekaterina Koptelova, Sh. A. Ehgamberdiev, David Hiriart, Merja Tornikoski, J. A. Acosta-Pulido, D. Carosati, Mauro Dolci, G. M. Richter, Ann E. Wehrle, A. I. Gonzále, I. Agudo, T. M. Carleton, José L. Gómez, I. M. McHardy, Alan P. Marscher, I. S. Troitsky, I. Puerto-Gimenez, M. G. Nikolashvili, E. N. Kopatskaya, Paolo Leto, Corrado Trigilio, G. Umana, N. Smith, T. Sakamoto, Kari Nilsson, Omar M. Kurtanidze, Wen Ping Chen, Sofia O. Kurtanidze, Raúl Mújica, A. Bueno, Filippo D'Ammando, C. M. Raiteri, L. O. Takalo, Valeri M. Larionov, Brian W. Taylor, M. I. Carnerero, Sh. Holikov, A. A. Arkharov, N. V. Efimova, Joni Tammi, Manasvita Joshi, Paul S. Smith, M. Villata, Andrei Berdyugin, Erika Benítez, U. Bach, Dmitry A. Blinov, Hugh D. Aller, V. A. Hagen-Thorn, M. F. Aller, Elina Lindfors, Carla Buemi
Publikováno v:
SCOPUS00046361-2012-545-SID84865714647
The quasar-type blazar 4C 38.41 (B3 1633+382) experienced a large outburst in 2011, which was detected throughout the entire electromagnetic spectrum. We present the results of low-energy multifrequency monitoring by the GASP project of the WEBT cons
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1fe4d4c910669777189195f511779e25
http://hdl.handle.net/20.500.12386/32898
http://hdl.handle.net/20.500.12386/32898
Autor:
Christopher W. Stubbs, J. N. Heasley, Chien-Hsiu Lee, Robert Jedicke, Robert H. Lupton, Paul A. Price, Gerard Anthony Luppino, Tommy Grav, C. K. Huang, W. P. Chen, Richard J. Wainscoat, Peter M. Onaka, William S. Burgett, Mengchun Tsai, R. P. Kudritzki, K. C. Chambers, Klaus W. Hodapp, J. S. Morgan, John L. Tonry, C. H. Tang, Mark E. Huber, Ping Wang, Nick Kaiser, Neelam Panwar, Nigel Metcalfe, H. Flewelling, Peter W. Draper, E. A. Magnier, Bertrand Goldman, Christopher Waters, Chien-Cheng Lin, W. E. Sweeney, Ashwani Pandey, David G. Monet
Publikováno v:
Astrophysical journal, 2014, Vol.784(1), pp.57 [Peer Reviewed Journal]
Membership identification is the first step to determine the properties of a star cluster. Low-mass members in particular could be used to trace the dynamical history, such as mass segregation, stellar evaporation, or tidal stripping, of a star clust