2003ApJ...587L.109S


Query : 2003ApJ...587L.109S

2003ApJ...587L.109S - Astrophys. J., 587, L109-L112 (2003/April-3)

Evidence for grain growth in the protostellar disks of Orion.

SHUPING R.Y., BALLY J., MORRIS M. and THROOP H.

Abstract (from CDS):

We present a Brα (λ=4.05 µm) image of the largest silhouette proplyd in Orion (114-426) using the facility near-IR spectrometer NIRSPEC at the Keck Observatory. This is the longest wavelength observation of a silhouette disk to date. The diameter of the disk at 4 µm is only marginally smaller than that observed in the optical with the Hubble Space Telescope. This may be the first signature of chromatic extinction for the translucent outer edges of the disk, suggesting that the near-IR opacity is dominated by processed grains with typical sizes greater than 1.9 µm, but not ≫4 µm.

Abstract Copyright: ∼

Journal keyword(s): Stars: Circumstellar Matter - ISM: Dust, Extinction - Stars: Formation - Stars: Pre-Main-Sequence

Simbad objects: 9

goto Full paper

goto View the references in ADS

Number of rows : 9
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 V* V1213 Tau Or* 04 31 37.5055489536 +18 12 24.383952396           K7 605 0
2 NAME Taurus Complex SFR 04 41.0 +25 52           ~ 4971 0
3 V* GM Aur Or* 04 55 10.9815576936 +30 21 59.373771876 14.59 13.351 12.242 11.798   K3Ve 797 0
4 NAME Orion Nebula Cluster OpC 05 35.0 -05 29           ~ 2514 0
5 COUP 419 Y*O 05 35 11.320 -05 24 26.54           M0 61 0
6 M 42 HII 05 35 16.8 -05 23 15           ~ 4411 0
7 NAME Ori A MoC 05 38 -07.1           ~ 3187 0
8 NGC 2024 Cl* 05 41 43 -01 50.5           ~ 1198 1
9 HD 109573 TT* 12 36 01.0317461592 -39 52 10.220465388   5.786 5.774   5.81 A0V 684 1

To bookmark this query, right click on this link: simbad:objects in 2003ApJ...587L.109S and select 'bookmark this link' or equivalent in the popup menu