Zobrazeno 241 - 250
of 2 003
pro vyhledávání: '"Ho, Paul"'
Publikováno v:
In Asian Journal of Pharmaceutical Sciences January 2018 13(1):72-81
Publikováno v:
Astrophys.J. 624 (2005) L49-L52
We present high resolution (0.''12 x 0.''079) observations of the ultracompact HII region G10.6-0.4 in 23 GHz radio continuum and the NH3(3,3) line. Our data show that the infall in the molecular material is largely spherical, and does not flatten in
Externí odkaz:
http://arxiv.org/abs/astro-ph/0410604
Publikováno v:
Astrophys.J. 616 (2004) L47-L50; Erratum-ibid. 617 (2004) L93
We used the Submillimeter Array to image the SiO maser emission in the $v=1$, \$J=5-4$ transition associated with the peculiar red supergiant VY Canis Majoris. We identified seven maser components and measured their relative positions and linear pola
Externí odkaz:
http://arxiv.org/abs/astro-ph/0408298
Publikováno v:
Astron.Astrophys. 426 (2004) 941-949
We present a detailed kinematical study and modeling of the emission of the molecular cores at ambient velocities surrounding IRAS 21391+5802, an intermediate-mass protostar embedded in IC 1396N. The high-density gas emission is found in association
Externí odkaz:
http://arxiv.org/abs/astro-ph/0407102
Publikováno v:
Astrophys.J. 610 (2004) L121-L124
We present sensitive 1.3 cm radio continuum observations of the region OMC1 South (OMC-1S) in Orion using the Very Large Array in its B configuration. We detect eleven radio sources clustered in a $30{''} \times 30{''}$ region, of which only three ha
Externí odkaz:
http://arxiv.org/abs/astro-ph/0407009
Publikováno v:
Astrophys.J.616:L1-L6,2004
The Submillimeter Array (SMA), a collaborative project of the Smithsonian Astrophysical Observatory (SAO) and the Academia Sinica Institute of Astronomy and Astrophysics (ASIAA), has begun operation on Mauna Kea in Hawaii. A total of eight 6-m telesc
Externí odkaz:
http://arxiv.org/abs/astro-ph/0406352
Publikováno v:
Astrophys.J. 616 (2004) L67-L70
We present observations of the CO 2-1 and 3-2 transitions toward the merging galaxies of NGC6090 with the Submillimeter Array (SMA) (The Submillimeter Array (SMA) is a joint project between the Smithsonian Astrophysical Observatory and the Academia S
Externí odkaz:
http://arxiv.org/abs/astro-ph/0405435
Autor:
Takakuwa, Shigehisa, Ohashi, Nagayoshi, Ho, Paul T. P., Qi, Chunhua, Wilner, David J., Zhang, Qizhou, Bourke, Tyler L., Hirano, Naomi, Choi, Minho, Yang, Ji
Publikováno v:
Astrophys.J. 616 (2004) L15-L18
We have imaged the circumstellar envelope around the binary protostar L1551 IRS 5 in CS (J=7-6) and 343 GHz continuum emission at ~ 3 arcsec resolution using the Submillimeter Array. The continuum emission shows an elongated structure (~ 220 x 100 AU
Externí odkaz:
http://arxiv.org/abs/astro-ph/0404346
Autor:
Iono, Daisuke, Ho, Paul T. P., Yun, Min S., Matsushita, Satoki, Peck, Alison B., Sakamoto, Kazushi
Publikováno v:
Astrophys.J. 616 (2004) L63-L66
New high resolution CO(3-2) interferometric map of the IR-bright interacting galaxy system VV114 observed with the Submillimeter Array (SMA) reveal a substantial amount of warm and dense gas in the IR-bright but optically obscured galaxy, VV114E, and
Externí odkaz:
http://arxiv.org/abs/astro-ph/0403429
Autor:
Anglada, Guillem, Rodriguez, Luis F., Osorio, Mayra, Torrelles, Jose M., Estalella, Robert, Beltran, Maria T., Ho, Paul T. P.
Publikováno v:
Astrophys.J. 605 (2004) L137-L140
We present Very Large Array observations at 7 mm of the sources IRAS 2A, IRAS 2B, MMS2, MMS3 and SVS 13, in the NGC1333 region. SVS 13 is a young close binary system whose components are separated by 65 AU in projection. Our high angular resolution o
Externí odkaz:
http://arxiv.org/abs/astro-ph/0403151