... but are warmed by that visible light and so radiate in the IR visible light image IR light image mosaic IR stars in Orion IR star DC303.8-14.2 visible light ...
Brief introduction of the SMA Project. Star formation and disk ... Geometry: compact, disklike structures. Kinematics: Kepler motions. LAB, France 07.01.2009 ...
YSO/PMS disk types, time-scales and evolution Luke Thomas Maud ESAC Trainee 2009 Bruno Merin Herschel Science centre (Supervisor) Herv Bouy Herschel ...
Can space-filling isotropic turbulence be driven by needles (jets), or balloons (outflows) ... Explore time-decaying Jets/WAW outflow evolution (Bertout et al 96) ...
THE EFFECT OF THE LSO/YSO CONCENTRATIONS RATIO ON THE IMAGING CHARACTERISTICS UNDER MAMMOGRAPHIC CONDITIONS Anastasios C. Konstantinidis1, Panayiotis F. Liaparinos1 ...
T Tauri Stars. Can YSO's Effect Your Horoscope? Presenter: Paul Edmon. 12-05-05. Astronomy 4001 ... Time scales to reach the Zero Age Main Sequence (ZAMS) vary ...
Hiro Takami1, Tomoyuki Kudo2,3, Yoshiko Okamoto3, Motohide ... (Grady et al. 2001) (Clampin et al. 2003) FN Tau. HD 142527. AB Aur. HD 100546. HD 141569A ...
Instituto de Astrof sica de Andaluc a (CSIC) 'Remembering Lucas Lara'- 6 March 2007 ... 100 durante varias decenas de minutos proviene de una regi n puntual 10 Rsch ...
(HST Public Pictures) X-ray binary (SS 433, Courtesy of Amy J. Mioduszewski) Nearby AGN ... UV/X-ray excitation scenarii would not give momentum flux as a T Tauri star ...
Hard X-ray view of nearby Star Forming Regions S. Sciortino INAF-Osservatorio Astronomico di Palermo COUP X-ray emission from (low-mass) YSOs Very X-ray luminous At 1 ...
... more massive than T Tau N (one of the brightest & most massive YSOs in Taurus!) How can this be? ... explain the observed characteristics of T Tau, and ...
Understanding the physics of accretion-ejection flows. is central to the understanding of ... Jet acceleration and collimation. Emission from shocks in YSO jets ...
HIGH VELOCITY JETS IN WATER-FOUNTAIN PRE-PLANETARY NEBULAE. Mark Claussen, NRAO. July 30, 2003 ... shocks seen in water maser proper motion studies. of YSO's. ...
Mechanisms for producing LS fields. Field at scale larger than that of turbulence ... Small PrM: stars and discs around NSs and YSOs. Here: non-helically ...
very X-ray sensitive. very FUV sensitive. not sensitive. very X-ray sensitive. slightly X-ray sensitive. Main formation reactions in YSO envelopes due to X-rays ...
Within the context of the Planck mission prepare for the use of HFI and LFI data ... emission of YSOs, in particular, investigating the influence of X-ray emission ...
FU Ori. FUor's are YSO's with significant circumstellar material. ... Observed frequency of FU Ori eruptions (last 50 years) is several times greater ...
On the role of stellar wind in MHD accretion-ejection structure. MPA ... 50% of YSOs (Millimeter and Near IR observation) 10% of Micro-quasar, quasar. Transport ...
Preparatory observations VLT - VLT-ISAAC survey of ~50 Class I YSO's ... SIRTF R~600 only at 10 mm = ground-based. high resolution in 3-5 mm range. Ophiuchus sources ...
Title: The Structures and Kinematics of Protoclusters Author: Trial User Last modified by: Trial User Created Date: 7/20/2003 6:07:28 AM Document presentation format
The Red MSX Source Survey. RMS Team: Stuart Lumsden, Rene Oudmaijer, James ... Toby Moore, James Allsopp (Liverpool JMU) Cormac Purcell, Michael Burton (UNSW) ...
Title: No Slide Title Author: mkuchner Last modified by: mkuchner Created Date: 5/20/2002 12:52:32 AM Document presentation format: On-screen Show Company
Software Modelling of IFU Spectrometers Nuria P. F. Lorente UK Astronomy Technology Centre Royal Observatory, Edinburgh, UK Alistair C. H. Glasse, Gillian S. Wright ...
Title: Can extra-solar planets be detected with mm interferometry? Author: Vincent Minier Last modified by: Vincent Minier Created Date: 12/4/2001 4:30:19 AM
From Pre-Stellar Cores to Protostars: The Initial Conditions of Star Formation Andre P., Ward-Thompson D., Barsony M., 2000, in Protostars and Planets IV, ed. V ...
Magnetic field rooted at star surface are resposible for flaring ... Dominating cosmic ray ionization ~4000AU (Krolic & Kallman 1983) Ionization mechanism ...
Famous Eagle. Nebula image. Cool dark clouds. are close to ... AGB (Asymptotic Giant Branch) These differ in position on H-R diagram and in. interior structure ...
Molecular Surveys of the Disks Encircling T Tauri/Herbig Ae Stars Geoffrey A. Blake CalTech Chemistry as a Diagnostic of Star Formation Waterloo, Canada 23Aug2002
Title: Slide 1 Author: Gary Last modified by: Gary Document presentation format: Custom Other titles: Gill Sans ProN W3 Arial Calibri Verdana Comic ...
Deep near-infrared observations of high mass Galactic star forming regions ... 1 Tata Institute of Fundamental Research, Mumbai (Bombay) 400 005, India (ojha ...
High-Mass Star Formation UKIDSS & GLIMPSE Views. Melvin Hoare ... Robitaille et al. Model Fitter results to 2MASS, MSX, TIMMI2, IRAS. The CORNISH Survey ...