Results 51 to 60 of about 4,221 (136)

Detections of CO Molecular Gas in 24um-Bright ULIRGs at z~2 in the Spitzer First Look Survey [PDF]

open access: yes, 2010
We present CO observations of 9 ULIRGs at z~2 with S(24\mu m)>1mJy, previously confirmed with the mid-IR spectra in the Spitzer First Look Survey. All targets are required to have accurate redshifts from Keck/GEMINI near-IR spectra.
A. Omont   +49 more
core   +3 more sources

Numerical Simulations of Radiatively-Driven Dusty Winds [PDF]

open access: yes, 2013
[abridged] Radiation pressure on dust grains may be an important mechanism in driving winds in a wide variety of astrophysical systems. However, the efficiency of the coupling between the radiation field and the dusty gas is poorly understood in ...
Krumholz, Mark R., Thompson, Todd A.
core   +1 more source

Hidden in plain sight: a massive, dusty starburst in a galaxy protocluster at z=5.7 in the COSMOS field [PDF]

open access: yes, 2018
We report the serendipitous discovery of a dusty, starbursting galaxy at $z=5.667$ (hereafter called CRLE) in close physical association with the "normal" main-sequence galaxy HZ10 at $z=5.654$. CRLE was identified by detection of [CII], [NII] and CO(2-1)
Capak, Peter L.   +9 more
core   +3 more sources

Penetapan Kadar Capsaicin Beberapa Jenis Cabe (Capsicum SP) Di Indonesia [PDF]

open access: yes, 2013
Capsaicin – the major active principle in chillies is an alkaloid, which cause the ‘hot' sensation when contact with the skin and muscous membrane. At least twenty varieties of consumable chillies known in Indonesia, and each of them has different degree
Sumpena, U. (U)
core  

Constraints on Stirring and Dissipation of MHD Turbulence in Molecular Clouds

open access: yes, 2001
We discuss constraints on the rates of stirring and dissipation of MHD turbulence in molecular clouds. Recent MHD simulations suggest that turbulence in clouds decays rapidly, thus providing a significant source of energy input, particularly if driven at
Chandrasekhar S.   +6 more
core   +1 more source

Radio Continuum and Star Formation in CO-rich Early Type Galaxies

open access: yes, 2007
In this paper we present new high resolution VLA 1.4 GHz radio continuum observations of five FIR bright CO-rich early-type galaxies and two dwarf early-type galaxies.
Braun R.   +14 more
core   +1 more source

Kinematic Distances to Molecular Clouds identified in the Galactic Ring Survey [PDF]

open access: yes, 2009
Kinematic distances to 750 molecular clouds identified in the 13CO J=1-0 Boston University-Five College Radio Astronomy Observatory Galactic Ring Survey (BU-FCRAO GRS) are derived assuming the Clemens rotation curve of the Galaxy.
Alexis Johnson   +43 more
core   +4 more sources

Elliptical Galaxy in the Making: The Dual Active Galactic Nuclei and Metal-enriched Halo of Mrk 273 [PDF]

open access: yes, 2019
A systematic analysis of the X-ray emission from the nearby ultraluminous infrared galaxy Mrk 273 was carried out by combining new 200 ksec Chandra data with archived 44 ksec data.
Iwasawa, Kazushi   +9 more
core   +2 more sources

Spatial distribution of far infrared emission in spiral galaxies I. Relation with radio continuum emission

open access: yes, 1997
We use high resolution IRAS and 20 cm radio continuum (RC) images of a sample of 22 spiral galaxies to study the correlation between the far infra-red (FIR) and RC emissions within the galactic disks.
Mayya, Y. D., Rengarajan, T. N.
core   +1 more source

Evidence for episodic warm outflowing CO gas from the intermediate mass young stellar object IRAS 08470-4321 [PDF]

open access: yes, 2010
We present a R=10,000 M-band spectrum of LLN19 (IRAS 08470-4321), a heavily embedded intermediate-mass young stellar object located in the Vela Molecular Cloud, obtained with VLT-ISAAC.
Dartois, E.   +3 more
core   +2 more sources

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