Zobrazeno 1 - 10
of 229
pro vyhledávání: '"Rugel, M"'
Autor:
Medina, S. -N. X., Dzib, S. A., Urquhart, J. S., Yang, A. Y., Brunthaler, A., Menten, K. M., Wyrowski, F., Cotton, W. D., Cheema, A., Dokara, R., Gong, Y., Khan, S., Nguyen, H., Ortiz-Leon, G. N., Rugel, M. R., Veena, V. S., Beuther, H., Csengeri, T., Pandian, J. D., Roy, N.
Publikováno v:
A&A 689, A196 (2024)
The GLOSTAR survey studies star formation with the VLA and the Effelsberg 100m telescope in the Galactic plane (-2d
Externí odkaz:
http://arxiv.org/abs/2407.12585
Autor:
Khan, S., Rugel, M. R., Brunthaler, A., Menten, K. M., Wyrowski, F., Urquhart, J. S., Gong, Y., Yang, A. Y., Nguyen, H., Dokara, R., Dzib, S. A., Medina, S. -N. X., Ortiz-León, G. N., Pandian, J. D., Beuther, H., Veena, V. S., Neupane, S., Cheema, A., Reich, W., Roy, N.
Publikováno v:
A&A 689, A81 (2024)
Studies of Galactic HII regions are of crucial importance for studying star formation and the evolution of the interstellar medium. Gaining an insight into their physical characteristics contributes to a more comprehensive understanding of these phen
Externí odkaz:
http://arxiv.org/abs/2407.05770
Autor:
Yang, A. Y., Dzib, S. A., Urquhart, J. S., Brunthaler, A., Medina, S. -N. X., Menten, K. M., Wyrowski, F., Ortiz-León, G. N., Cotton, W. D., Gong, Y., Dokara, R., Rugel, M. R., Beuther, H., Pandian, J. D., Csengeri, T., Veena, V. S., Roy, N., Nguyen, H., Winkel, B., Ott, J., Carrasco-Gonzalez, C., Khan, S., Cheema, A.
Publikováno v:
A&A 680, A92 (2023)
As part of the GLOSTAR (GLObal view of STAR formation in the Milky Way) survey, we present the high-resolution continuum source catalog for the regions (l = 2-28, 36-40, 56-60, &|b|<1.0), observed with the Karl G. Jansky Very Large Array (VLA) in its
Externí odkaz:
http://arxiv.org/abs/2310.09777
Autor:
Syed, J., Beuther, H., Goldsmith, P. F., Henning, Th., Heyer, M., Klessen, R. S., Stil, J. M., Soler, J. D., Anderson, L. D., Urquhart, J. S., Rugel, M. R., Johnston, K. G., Brunthaler, A.
Stars form in the dense interiors of molecular clouds. The dynamics and physical properties of the atomic interstellar medium (ISM) set the conditions under which molecular clouds and eventually stars will form. It is, therefore, critical to investig
Externí odkaz:
http://arxiv.org/abs/2310.02077
Autor:
Gong, Y., Du, F. J., Henkel, C., Jacob, A. M., Belloche, A., Wang, J. Z., Menten, K. M., Yang, W., Quan, D. H., Bop, C. T., Ortiz-León, G. N., Tang, X. D., Rugel, M. R., Liu, S.
Publikováno v:
A&A 679, A39 (2023)
Protonated hydrogen cyanide, HCNH$^{+}$, plays a fundamental role in astrochemistry because it is an intermediary in gas-phase ion-neutral reactions within cold molecular clouds. However, the impact of the environment on the chemistry of HCNH$^{+}$ r
Externí odkaz:
http://arxiv.org/abs/2308.15521
Autor:
Gong, Y., Ortiz-León, G. N., Rugel, M. R., Menten, K. M., Brunthaler, A., Wyrowski, F., Henkel, C., Beuther, H., Dzib, S. A., Urquhart, J. S., Yang, A. Y., Pandian, J. D., Dokara, R., Veena, V. S., Nguyen, H., Medina, S. -N. X., Cotton, W. D., Reich, W., Winkel, B., Müller, P., Skretas, I., Csengeri, T., Khan, S., Cheema, A.
Publikováno v:
A&A 678, A130 (2023)
Cygnus X is one of the closest and most active high-mass star-forming regions in our Galaxy, making it one of the best laboratories for studying massive star formation. As part of the GLOSTAR Galactic plane survey, we performed large scale simultaneo
Externí odkaz:
http://arxiv.org/abs/2308.00993
Autor:
Padmanabh, P. V., Barr, E. D., Sridhar, S. S., Rugel, M. R., Damas-Segovia, A., Jacob, A. M., Balakrishnan, V., Berezina, M., Bernadich, M. C. i, Brunthaler, A., Champion, D. J., Freire, P. C. C., Khan, S., Klöckner, H. -R., Kramer, M., Ma, Y. K., Mao, S. A., Men, Y. P., Menten, K. M., Sengupta, S., Krishnan, V. Venkatraman, Wucknitz, O., Wyrowski, F., Bezuidenhout, M. C., Buchner, S., Burgay, M., Chen, W., Clark, C. J., Künkel, L., Nieder, L., Stappers, B., Legodi, L. S., Nyamai, M. M.
Galactic plane radio surveys play a key role in improving our understanding of a wide range of astrophysical phenomena. Performing such a survey using the latest interferometric telescopes produces large data rates necessitating a shift towards fully
Externí odkaz:
http://arxiv.org/abs/2303.09231
Autor:
Dokara, R., Gong, Y., Reich, W., Rugel, M., Brunthaler, A., Menten, K., Cotton, W., Dzib, S., Khan, S., Medina, S., Nguyen, H., Ortiz-León, G., Urquhart, J., Wyrowski, F., Yang, A., Anderson, L. D., Beuther, H., Csengeri, T., Müller, P., Ott, J., Pandian, J. D., Roy, N.
Publikováno v:
A&A 671, A145 (2023)
Context. While over 1000 supernova remnants (SNRs) are estimated to exist in the Milky Way, only less than 400 have been found to date. In the context of this apparent deficiency, more than 150 SNR candidates were recently identified in the D-configu
Externí odkaz:
http://arxiv.org/abs/2211.13811
Autor:
Dzib, S. A., Yang, A. Y., Urquhart, J. S., Medina, S. -N. X., Brunthaler, A., Menten, K. M., Wyrowski, F., Cotton, W. D., Dokara, R., Ortiz-León, G. N., Rugel, M. R., Nguyen, H., Gong, Y., Chakraborty, A., Beuther, H., Billington, S. J., Carrasco-Gonzalez, C., Csengeri, T., Hofner, P., Ott, J., Pandian, J. D., Roy, N., Yanza, V.
Publikováno v:
A&A 670, A9 (2023)
As part of the GLOSTAR survey we have used the VLA in its B-configuration to observe the part of the Galactic plane between longitudes of 28d and 36d and latitudes from -1d to +1d at the C-band (4--8 GHz). To reduce the contamination of extended sour
Externí odkaz:
http://arxiv.org/abs/2210.00560
Autor:
Nguyen, H., Rugel, M. R., Murugeshan, C., Menten, K. M., Brunthaler, A., Urquhart, J. S., Dokara, R., Dzib, S. A., Gong, Y., Khan, S., Medina, S-N. X., Ortiz-Leon, G. N., Reich, W., Wyrowski, F., Yang, A. Y., Beuther, H., Cotton, W. D., Pandian, J. D.
Publikováno v:
A&A 666, A59 (2022)
Class II methanol (CH$_{3}$OH) masers are amongst the clearest signposts of recent high-mass star formation (HMSF). A complete catalogue outlines the distribution of star formation in the Galaxy, the number of young star-forming cores, and the physic
Externí odkaz:
http://arxiv.org/abs/2207.10548