نتایج جستجو برای: iram

تعداد نتایج: 656  

Journal: :Epj Web of Conferences 2022

In the context of CALYPSO IRAM-PdBI Lai•ge Program we performed first statistical survey protostellar jets by analysing molecular emission in a sample 21 protostars covering broad range internal luminosities (L int from 0.035 L ⊙ to 47 ). We find that outflow phenomenon is ubiquitous our protostars, with wide-angle outflows detected CO (2 - 1) all sources, and high-velocity collimated SiO (5-4)...

Journal: :The Astrophysical Journal 2019

Journal: :Astronomy and Astrophysics 2022

We present the results of millimetre-wave spectroscopic and continuum observations comet C/2020 F3 (NEOWISE) undertaken with Institut de RadioAstronomie Millimétrique (IRAM) 30-m NOrthern Extended Millimeter Array (NOEMA) telescopes on 22, 25–27 July, 7 August 2020. Production rates HCN, HNC, CH 3 OH CS, H 2 CO, CN, S, CO were determined upper limits six other species. The shows abundances with...

Journal: :Publications of the Astronomical Society of the Pacific 2008

2015
N. P. H. Nesvadba D. Guery T. McKenzie S. König G. Petitpas H. Dole B. Frye I. Flores-Cacho L. Montier M. Negrello A. Beelen F. Boone D. Dicken G. Lagache E. Le Floc’h B. Altieri M. Béthermin R. Chary G. de Zotti M. Giard R. Kneissl M. Krips

We present an analysis of CO spectroscopy and infrared-to-millimetre dust photometry of 11 bright far-infrared/submillimetre sources discovered through a combination of the Planck all-sky survey and follow-up Herschel-SPIRE imaging – “Planck’s Dusty Gravitationally Enhanced subMillimetre Sources.” Each source has a spectroscopic redshift z = 2.2–3.6 from a blind redshift search with EMIR at the...

2009
N. P. H. Nesvadba R. Neri C. De Breuck M. D. Lehnert D. Downes F. Walter A. Omont F. Boulanger N. Seymour

We report the detection of luminous CO(3–2) line emission in the halo of the z=2.6 radio galaxy (HzRG) TXS0828+193, which has no detected counterpart at optical to mid-infrared wavelengths implying a stellar mass . few×10 M⊙ and relatively low star-formation rates. With the IRAM PdBI we find two CO emission line components at the same position at ∼80 kpc distance from the HzRG along the axis of...

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