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GGD 7 IR Stellar Group t

GGD 7 IR Stellar Group t

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Fig. 5.-J vs. J − H color magnitude diagrams for young

Figure 22.

Age analysis within individual stellar clusters. Examples are given for six clusters; the complete

YOUNG STELLAR OBJECT VARIABILITY (YSOVAR): LONG TIMESCALE VARIATIONS IN THE MID-INFRARED - IOPscience

Comparison between the far-IR/radio (IRAS 100 μ m/VLA 2

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Figure 10.

YOUNG STELLAR OBJECT VARIABILITY (YSOVAR): LONG TIMESCALE VARIATIONS IN THE MID-INFRARED - IOPscience

Figure 15.

The young stellar objects GGD 4. (Field size 6.7´ × 6.7´. Image size 145 kb.)

Comparison between the mid-IR/radio (MSX 21 μ m/VLA 2

YOUNG STELLAR OBJECT VARIABILITY (YSOVAR): LONG TIMESCALE VARIATIONS IN THE MID-INFRARED - IOPscience

YOUNG STELLAR OBJECT VARIABILITY (YSOVAR): LONG TIMESCALE VARIATIONS IN THE MID-INFRARED - IOPscience

The radial distribution of stellar density. Fig. 2. JH

Gradient scales in the MYStIX (red), SFiNCs (green), and MYStIX

IR colour–magnitude diagram of UCH ii regions: comparison between MSX mid-IR

Figure 10. Fraction of systems with ∆RVmax> 10 km s −1 in

Stellar parameters derived from SED fit

Radial density distribution of stellar objects: relative classes (b)

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Same as Fig. 5, but for Sh2-235B Cluster, BDSB 73,

Extremely Young Stellar Objects in L1551. The Lynds 1551 (L1551) dark cloud region contains several very young low-mass stellar objects in the process of ...

Atlas Image mosaic of IRAS 17244-3536, which appears to be a region of high gas density and a source of CS molecular emission (Chan, Henning, & Streyer 1996 ...

YOUNG STELLAR OBJECT VARIABILITY (YSOVAR): LONG TIMESCALE VARIATIONS IN THE MID-INFRARED - IOPscience

Fig. 3. Position of κ And A in a color-magnitude diagram (. +7

Fig. 2.-Spitzer and CoRoT data for two stars from Table 1 (

T Tauri

Fig. 11.— Histogram of the timescale τ in the auto-correlation function

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Fig. 8. A sample of Class 0/I sources showing their similarity at

GGD 27

YOUNG STELLAR OBJECT VARIABILITY (YSOVAR): LONG TIMESCALE VARIATIONS IN THE MID-INFRARED - IOPscience

Table 2 . Physical parameters of the EPIC212521166 system

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The young stellar population in the Serpens Cloud Core: An ISOCAM survey

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GGD 4

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MSX band E images of UCH ii regions. Each field covers a field of view

Comparison between the broad-band, mid-IR filter profiles of MSX, of

Comparison between the far-IR/radio (IRAS 100 μ m/VLA 6

Angular distribution of the decontaminated stellar content for FSR 784, Sh2-235 Cluster,

Cluster stacking analysis using standardized variables. Standardized age as a function of standardized radial distance

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Same as Fig. A1.

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7.— J vs. J − K s for the sample.

Young Stellar Groups, Runaway Stars, and Pulsars

Figure 19.

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7.-Radial profile (as indicated in Fig. 4) through

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T Tauri stars

Simulated application of the MST method. Upper-left panel: the spatial distribution of

When the shell is driven by the pressure of the hot bubble of shocked stellar wind, the radius of the shell, Rsh, increases with time as (Castor et al.

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YSOVAR: Mid-infrared Variability Among YSOs in the Star Formation Region GGD 12-15

Continuous Improvement

Parameters of the stellar distribution model.

Atlas ...

Figure 7. Left panel: FUV luminosity vs. age for young low-mass

Picture

Position–velocity plots centred on the 2.122-μm emission line. Contours measure 3

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ZD60 comparison edge 1-1

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2004, AAS, 204, 41.02 ...

Download Down & Dirty - Heaven Sent [Unofficial EP] (2018)

First 2Myr of the dynamical evolution of a sample cluster with N=250 and a

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Mid-IR image of the centre of the galaxy, with the Quintuplet stars as the brightest source to the left of the centre (and 2nd inset)

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Same as Fig

Cumulative semi-major axis for Oort clouds for various Hernquist clusters

JPG IMG_9057.

The ...

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Eta Carinae - Hubble composite of Eta Carinae showing the unusual emission spectrum (near-