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[PDF] Top 20 A source of extended HCO+ emission in young stellar objects

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A source of extended HCO+ emission in young stellar objects

A source of extended HCO+ emission in young stellar objects

... simplifications have been made. First, the abundances that have been inferred from the observations, and which we have attempted to model, have been deduced on the assumption of a specific dynamical scenario (spherically ... See full document

8

The RMS survey: ammonia mapping of the environment of massive young stellar objects

The RMS survey: ammonia mapping of the environment of massive young stellar objects

... We find upon examination of the single component sources that the broad line widths are often found to be at the apex of a cone shape that extends to the edges of the clump, and in a smaller number of cases this is ... See full document

25

VISION   Vienna survey in Orion III  Young stellar objects in Orion A

VISION Vienna survey in Orion III Young stellar objects in Orion A

... very young, either at the end of the embedded protostellar phase or at the beginning of the disk-dominated PMS phase, since they had not enough time to disperse similarly as the Class II YSO ... See full document

39

Main sequence stars masquerading as young stellar objects in the central molecular zone

Main sequence stars masquerading as young stellar objects in the central molecular zone

... from young stellar objects ...μm emission is up to an order of magnitude higher than the value estimated from methods based on diffuse emission (such as free–free ...evolved ... See full document

11

Simulating radio emission from low mass stars

Simulating radio emission from low mass stars

... gyrosynchrotron emission alone should be L n , R = 10 ...tron emission is a negligible contribution to the total radio fl ux from V374 ...from young stellar ...radio emission through ECM ... See full document

8

The palomar transient factory orion project: eclipsing binaries and young stellar objects

The palomar transient factory orion project: eclipsing binaries and young stellar objects

... Any source detection with a flagged pixel within its photometry aperture is rejected and does not pass through the ...photometry. Source detection and aperture photome- try are performed using the IDL ... See full document

35

Herschel Hi-GAL imaging of massive young stellar objects

Herschel Hi-GAL imaging of massive young stellar objects

... structures) emission to allow an investigation of their extended ...sampled objects, between two and four point sources were detected at 8 µm in the Galactic Legacy Infrared Midplane Survey ... See full document

10

Lights and shadows :  multi wavelength analysis of young stellar objects and their protoplanetary discs

Lights and shadows : multi wavelength analysis of young stellar objects and their protoplanetary discs

... a source whose maximum emission peaks at wavelength λ, and does not include the contribution to that emission, at the same wavelength, from colder or hotter ...a source emitting at 850 ...disc ... See full document

257

Alves de Oliveira, Catarina
  

(2008):


	Near infrared variability phenomena in young stellar objects.


Dissertation, LMU München: Fakultät für Physik

Alves de Oliveira, Catarina (2008): Near infrared variability phenomena in young stellar objects. Dissertation, LMU München: Fakultät für Physik

... important source of contamination given the faint magnitude limits of the ...9 objects in the ρ Ophiuchi field, compared to the candidate-member sample of ... See full document

152

Outflows from young stellar objects: the case of DG Tauri

Outflows from young stellar objects: the case of DG Tauri

... presence of forming stars before they are revealed. Outflows may modify the structure of protostellar discs (Combet & Ferreira 2008), affect the penetration of ionizing particles and stellar radiation into the ... See full document

217

A model for (quasi )periodic multi wavelength photometric variability in young stellar objects

A model for (quasi )periodic multi wavelength photometric variability in young stellar objects

... rotating young stellar objects ( YSOs ) with hot spots in their atmospheres, inner disk warps, and other three-dimensional effects in the nearby circumstellar ...creates stellar hot spots upon ... See full document

15

AKARI observations of ice absorption bands towards edge-on young stellar objects

AKARI observations of ice absorption bands towards edge-on young stellar objects

... Young stellar objects have a complicated structure: a protostar, circumstellar disk, envelope, and outflow ...some objects might be accompanied by either ambient or fore- ground ...light ... See full document

12

Main-sequence stars masquerading as Young Stellar Objects in the central molecular zone

Main-sequence stars masquerading as Young Stellar Objects in the central molecular zone

... the stellar flux in the infrared ...whether objects not seen at wavelength longer than 24 µm may not be as young as 1 Myr (as assumed by Yusef-Zadeh et ...a source is a YSO or not, its size at ... See full document

12

The Early History of Stellar Spin: the Theory of Accretion onto Young Stellar Objects

The Early History of Stellar Spin: the Theory of Accretion onto Young Stellar Objects

... The key idea is that the shaking up of the stellar photosphere in the neighbourhood of the accretion column would launch waves propagating over the photosphere. Those regions with open magnetic field lines would ... See full document

12

The Red MSX Source Survey: The Massive Young Stellar Population of Our Galaxy

The Red MSX Source Survey: The Massive Young Stellar Population of Our Galaxy

... of young massive ...μm emission than 14 μm emission (suggestive of strong polycyclic aromatic hydrocarbon, PAH, emission commonly seen around H ii regions, but excluded from our color ... See full document

18

Realistic ionizing fluxes for young stellar populations from 0.05 to 2 ZÔ

Realistic ionizing fluxes for young stellar populations from 0.05 to 2 ZÔ

... of young stellar populations depends on the accuracy of the model atmospheres and evolutionary tracks for massive ...input stellar param- eters to reflect current values available in the ... See full document

21

Extremely red stellar objects revealed by IPHAS

Extremely red stellar objects revealed by IPHAS

... red stellar objects extracted from the point-source catalogue of the INT Photometric Hα Survey (IPHAS) of the northern galactic ...these objects have no previous ...these objects traces ... See full document

19

Astrophysical properties of LINER galaxies

Astrophysical properties of LINER galaxies

... X-ray source is thought to lie close to the MBH and this illuminates an optically thick, geometrically thin accretion ...X-ray emission and is thought to be the origin of the “Big Blue Bump” (BBB) and the ... See full document

236

TEXES observations of M supergiants: dynamics and thermodynamics of wind acceleration

TEXES observations of M supergiants: dynamics and thermodynamics of wind acceleration

... As one moves away from the star, the filling factor of hot chromospheric plasma decreases, and hence the difference between the mean temperature inferred from the VLA radio interferometry and the bulk gas temperature ... See full document

79

On the Origin of Mass and Angular Momentum of Stellar Objects

On the Origin of Mass and Angular Momentum of Stellar Objects

... projection breaks time reversal symmetry. Therefore there are only leptons with negative e charge with its neu- trinos in the 4D space time, and thus the universe does not contain anti-matter symmetry. Incidentally the ... See full document

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