Zobrazeno 1 - 6
of 6
pro vyhledávání: '"Rohit Dokara"'
Autor:
H. Nguyen, S.-N. X. Medina, Karl M. Menten, S. J. Billington, W. Reich, J. D. Pandian, Gisela N. Ortiz-León, C. Murugeshan, Rohit Dokara, Timea Csengeri, Friedrich Wyrowski, James Urquhart, Carlos Carrasco-González, Y. Gong, Peter Müller, Michael Rugel, Andreas Brunthaler, S. A. Dzib, Benjamin Winkel, W. D. Cotton, A. Y. Yang, Henrik Beuther, Nirupam Roy
Surveys of the Milky Way at various wavelengths have changed our view of star formation in our Galaxy considerably in recent years. In this paper we give an overview of the GLOSTAR survey, a new survey covering large parts (145 square degrees) of the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b76d10a8a5ad2bda5155e3cfb4c2b844
http://arxiv.org/abs/2106.00377
http://arxiv.org/abs/2106.00377
Autor:
Andreas Brunthaler, W. D. Cotton, Henrik Beuther, Timea Csengeri, Jagadheep D. Pandian, Michael Rugel, S. N. X. Medina, James Urquhart, Wolfgang Reich, Rohit Dokara, M. Schultheis, Nirupam Roy, A. Y. Yang, Jens Kauffmann, Karl M. Menten, H. Nguyen, Sergio A. Dzib, G. Nandakumar, Gisela N. Ortiz-León, Friedrich Wyrowski, Y. Gong, Thushara Pillai
The Central Molecular Zone (CMZ), a $\sim$200 pc sized region around the Galactic Centre, is peculiar in that it shows a star formation rate (SFR) that is suppressed with respect to the available dense gas. To study the SFR in the CMZ, young stellar
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6931e2219a60186c3537140bb0596ebf
http://arxiv.org/abs/2105.03212
http://arxiv.org/abs/2105.03212
Autor:
Carlos Carrasco-González, Timea Csengeri, Sergio A. Dzib, Gisela N. Ortiz-León, Michael Rugel, Rohit Dokara, S. N. X. Medina, Leroy Anderson, Friedrich Wyrowski, James Urquhart, S. J. Billington, Y. Gong, Andreas Brunthaler, Nirupam Roy, Wolfgang Reich, A. Y. Yang, Henrik Beuther, Karl M. Menten, C. H. R. Chen, W. D. Cotton
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 651, pp.A86. ⟨10.1051/0004-6361/202039873⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 651, pp.A86. ⟨10.1051/0004-6361/202039873⟩
Context. The properties of the population of Galactic supernova remnants (SNRs) are essential to our understanding of the dynamics of the interstellar medium (ISM) in the Milky Way. However, the completeness of the catalog of Galactic SNRs is expecte
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5b6aa7bbe2e3ea23c76c115e503748b4
https://hal.archives-ouvertes.fr/hal-03186198
https://hal.archives-ouvertes.fr/hal-03186198
Autor:
J. D. Pandian, Y. Gong, Andreas Brunthaler, Nirupam Roy, S. N. X. Medina, Gisela N. Ortiz-León, A. Y. Yang, Henrik Beuther, Wolfgang Reich, W. D. Cotton, Friedrich Wyrowski, Rohit Dokara, Karl M. Menten, Timea Csengeri, S. A. Dzib, James Urquhart, Michael Rugel, H. Nguyen, C. König
Publikováno v:
Astronomy & Astrophysics. 651:A87
The Cygnus X complex is covered by the Global View of Star Formation in the Milky Way (GLOSTAR) survey, an unbiased radio-wavelength Galactic plane survey, in 4--8 GHz continuum radiation and several spectral lines. The GLOSTAR survey observed the 6.
Autor:
Juan D. Soler, Michael Rugel, Jeroen M. Stil, Yuan Wang, Nirupam Roy, R. Shanahan, L. D. Anderson, Henrik Beuther, Rohit Dokara
Publikováno v:
The Astrophysical Journal
Anderson et al. (2017) identified seventy six candidate supernova remnants (SNRs) using data from The HI, OH, Recombination line survey of the Milky Way (THOR). The spectral index and polarization properties can help distinguish between SNRs and H II
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::989554f0880d460212509b2341a44c94
http://arxiv.org/abs/1808.06628
http://arxiv.org/abs/1808.06628
Autor:
Rohit Dokara, Nirupam Roy, Henrik Beuther, L. D. Anderson, Michael Rugel, Jeroen Stil, Yuan Wang, Juan D. Soler, Russel Shanahan
Publikováno v:
Astrophysical Journal; 10/10/2018, Vol. 866 Issue 1, p1-1, 1p