Zobrazeno 1 - 7
of 7
pro vyhledávání: '"Kumar, M. S. Nanda"'
Autor:
Arzoumanian, Doris, Arakawa, Sota, Kobayashi, Masato I. N., Iwasaki, Kazunari, Fukada, Kohei, Mori, Shoji, Hirai, Yutaka, Kunitomo, Masanobu, Kumar, M. S. Nanda, Kokubo, Eiichiro
Cylindrical molecular filaments are observed to be the main sites of Sun-like star formation, while massive stars form in dense hubs, at the junction of multiple filaments. The role of hub-filament configurations has not been discussed yet in relatio
Externí odkaz:
http://arxiv.org/abs/2303.15695
Autor:
Borissova, Jura, Bonatto, Charles, Kurtev, Radostin, Clarke, James R. A., Peñaloza, Francisco, Sale, Stuart E., Minniti, Dante, Alonso-García, Javier, Artigau, Étienne, Barbá, Rodolfo, Bica, Eduardo, Baume, Gustavo Luis, Catelan, Márcio, Chené, André-Nicolas, Dias, Bruno, Folkes, Stuart L., Froebrich, Dirk, Geisler, Doug, de Grijs, Richard, Hanson, Margaret M., Hempel, Maren, Ivanov, Valentin D., Kumar, M. S. Nanda, Lucas, Philip, Mauro, Francesco, Bidin, Christian Moni, Rejkuba, Marina, Saito, Roberto K., Tamura, Motohide, Toledo, Ignacio
VISTA Variables in the V\'{\i}a L\'actea (VVV) is one of the six ESO Public Surveys operating on the new 4-meter Visible and Infrared Survey Telescope for Astronomy (VISTA). VVV is scanning the Milky Way bulge and an adjacent section of the disk, whe
Externí odkaz:
http://arxiv.org/abs/1106.3045
Publikováno v:
Astrophys.J.598:1107-1111,2003
We present sub-arcsec (FWHM ~ 0.5") J, H, K and L' images of a young stellar cluster associated with a candidate massive protostar IRAS22134+5834. The observations reveal a centrally symmetric, flattened cluster enclosing a central dark region. The c
Externí odkaz:
http://arxiv.org/abs/astro-ph/0308275
Publikováno v:
Astron.Astrophys.344:L9-L12,1999
We report the detection of the H2 v=1-0 S(1) line at 2.122um, from RNO91 in the L43 dark cloud, which is known to be a T Tauri star surrounded by a 1700AU disk structure (containing ices) and a weak outflow. The non-detection of the H2 v=2-1 S(1) lin
Externí odkaz:
http://arxiv.org/abs/astro-ph/9903208
Autor:
Lucas, Philip William, Guo, Zhen, Contreras Pena, Carlos, Smith, Leigh Charles, Borissova, Jura, Kurtev, Radostin, Garcia, Javier Alonso, Minniti, Dante, Medina, Nicolas, Briceno, Cesar, Caratti o Graratti, Alessio, Froebrich, Dirk, Kumar, M. S. Nanda
This is the PowerPoint file associated used for the presentation.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3463b5c56bbad4d31fbdd572069f442a
Autor:
Sanchez-Monge, Alvaro, Cesaroni, Riccardo, Beltran, Maite, Kumar, M. S. Nanda, Stanke, Thomas, Zinnecker, Hans, Etoka, Sandra, Galli, Daniele, Hummel, Christian A., Luca Moscadelli, Preibisch, Thomas, Ratzka, Thorsten, Tak, Floris F. S., Vig, Sarita, Walmsley, C. Malcolm, Wang, Kuo-Song
Publikováno v:
NASA Astrophysics Data System
Protostars and Planets VI
Protostars and Planets VI
Recent theoretical models indicate that OB-type stars could form through disk-mediated accretion, like their low mass counterparts. However, on the observational side, circumstellar disks appear still elusive, especially around the most massive (prot
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::4af39684e02dec9572e93117dc43ef42
https://ui.adsabs.harvard.edu/#abs/2013prpl.conf1B045S
https://ui.adsabs.harvard.edu/#abs/2013prpl.conf1B045S
Publikováno v:
Astrophysical Journal; 9/1/2002, Vol. 576 Issue 1, p1-1, 1p
