Zobrazeno 1 - 10
of 58
pro vyhledávání: '"Furuya, R. S."'
Autor:
Hofner, P., Cesaroni, R., Kurtz, S., Rosero, V., Anderson, C., Furuya, R. S., Araya, E. D., Molinari, S.
We report 3 mm continuum, CH3CN(5-4) and 13CS(2-1) line observations with CARMA, in conjunction with 6 and 1.3 cm continuum VLA data, and 12 and 25 micron broadband data from the Subaru Telescope toward the massive proto-star IRAS18566+0408. The VLA
Externí odkaz:
http://arxiv.org/abs/1705.07203
Autor:
Moscadelli, L., Cesaroni, R., Sánchez-Monge, Á., Goddi, C., Furuya, R. S., Sanna, A., Pestalozzi, M.
Publikováno v:
A&A 558, A145 (2013)
We wish to investigate the structure, velocity field, and stellar content of the G16.59-0.05 high-mass star-forming region, where previous studies have established the presence of two almost perpendicular (NE-SW and SE-NW), massive outflows, and a ro
Externí odkaz:
http://arxiv.org/abs/1311.3499
Autor:
Li, J. J., Moscadelli, L., Cesaroni, R., Furuya, R. S., Xu, Y., Usuda, T., Menten, K. M., Pestalozzi, M., Elia, D., Schisano, E.
We used the Very Long Baseline Array (VLBA) and the European VLBI Network (EVN) to perform phase-referenced VLBI observations of the three most powerful maser transitions associated with the high-mass star-forming region G28.87+0.07: the 22.2 GHz H$_
Externí odkaz:
http://arxiv.org/abs/1201.3021
Aims: The main goal of this study is to perform a sub-arcsecond resolution analysis of the high-mass star formation region G19.61-0.23, both in the continuum and molecular line emission. While the centimeter continuum images will be discussed in deta
Externí odkaz:
http://arxiv.org/abs/1006.4353
The present paper focuses on the high-mass star-forming region G23.01-0.41. Methods: Using the VLBA and the EVN arrays, we conducted phase-referenced observations of the three most powerful maser species in G23.01-0.41: H2O at 22.2 GHz (4 epochs), CH
Externí odkaz:
http://arxiv.org/abs/1004.5578
Among the tracers of the earliest phases in the massive star formation process, methanol masers have gained increasing importance. The phenomenological distinction between Class I and II methanol masers is based on their spatial association with obje
Externí odkaz:
http://arxiv.org/abs/1004.3689
Using the OVRO, Nobeyama, and IRAM mm-arrays, we searched for ``disk''-outflow systems in three high-mass (proto)star forming regions: G16.59-0.05, G23.01-0.41, and G28.87+0.07. These were selected from a sample of NH3 cores associated with OH and H2
Externí odkaz:
http://arxiv.org/abs/0710.0029
This article reports first results of a long-term observational program aimed to study the earliest evolution of jet/disk systems in low-mass YSOs by means of VLBI observations of the 22.2 GHz water masers. We report here data for the cluster of low-
Externí odkaz:
http://arxiv.org/abs/astro-ph/0509663
Publikováno v:
Astrophys.J. 624 (2005) 827-831
Using the Owens Valley and Nobeyama Radio Observatory interferometers, we carried out an unbiased search for hot molecular cores and ultracompact UC HII regions toward the high-mass star forming region G19.61--0.23. In addition, we performed 1.2 mm i
Externí odkaz:
http://arxiv.org/abs/astro-ph/0501644
Publikováno v:
PASJ Letters vol.55, 2003 December 25 issue
We have conducted multi-epoch synthesis imaging of 2 and 3 millimeter (mm) continuum emission and near infrared K band 2.2 um imaging of a flare event in January 2003 that occurred on the young stellar object GMR-A which is suggested to be a weak-lin
Externí odkaz:
http://arxiv.org/abs/astro-ph/0310727