2017ApJ...834..115T


Query : 2017ApJ...834..115T

2017ApJ...834..115T - Astrophys. J., 834, 115-115 (2017/January-2)

Multi-epoch detections of water ice absorption in edge-on disks around Herbig Ae stars: PDS 144N and PDS 453.

TERADA H. and TOKUNAGA A.T.

Abstract (from CDS):

We report the multi-epoch detections of water ice in 2.8-4.2 µm spectra of two Herbig Ae stars, PDS 144N (A2 IVe) and PDS 453 (F2 Ve), which have an edge-on circumstellar disk. The detected water ice absorption is found to originate from their protoplanetary disks. The spectra show a relatively shallow absorption of water ice of around 3.1 µm for both objects. The optical depths of the water ice absorption are ∼0.1 and ∼0.2 for PDS 144N and PDS 453, respectively. Compared to the water ice previously detected in low-mass young stellar objects with an edge-on disk with a similar inclination angle, these optical depths are significantly lower. It suggests that stronger UV radiation from the central stars effectively decreases the water ice abundance around the Herbig Ae stars through photodesorption. The water ice absorption in PDS 453 shows a possible variation of the feature among the six observing epochs. This variation could be due to a change of absorption materials passing through our line of sight to the central star. The overall profile of the water ice absorption in PDS 453 is quite similar to the absorption previously reported in the edge-on disk object d216-0939, and this unique profile may be seen only at a high inclination angle in the range of 76°-80°.

Abstract Copyright: © 2017. The American Astronomical Society. All rights reserved.

Journal keyword(s): dust, extinction - evolution - infrared: ISM - protoplanetary disks - stars: individual: (PDS 144N, PDS 453) - stars: individual: (PDS 144N, PDS 453)

Simbad objects: 18

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Number of rows : 18
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* HK Tau B TT* 04 31 50.6002481212 +24 24 15.502558869           ~ 95 0
2 V* HV Tau C TT* 04 38 35.5125950280 +26 10 41.316576204         14.90 K6 110 0
3 NAME Orion Nebula Cluster OpC 05 35.0 -05 29           ~ 2514 0
4 V* V2151 Ori Or* 05 35 05.4087268512 -05 27 17.091689616   15.744 14.822 13.60 12.856 K5.5 61 1
5 COUP 460 Or* 05 35 12.0893467992 -05 19 24.753134964   15.5 20.92   15.581 M6 33 1
6 V* V2377 Ori Or* 05 35 21.5730392304 -05 09 38.823734232   15.1     15.509 K5 55 0
7 M 43 HII 05 35 31 -05 16.2           ~ 201 0
8 HD 120455 PM* 13 50 06.5085407184 -29 04 52.764518496   6.171 6.186     A0V 37 0
9 CD-25 11111A TT* 15 49 15.3256555968 -26 00 54.697740660   13.37 12.81 12.73   A5Ve 37 0
10 CD-25 11111 ** 15 49 15.3888 -26 00 52.452           A5Ve+A2IVe 30 0
11 CD-25 11111B TT* 15 49 15.5294156575 -26 00 50.039007268   13.37 12.81 14.02   A2IVe 35 0
12 HD 145127 * 16 10 09.8786833224 -24 34 56.713510524   6.66 6.64     A0V 48 0
13 NAME Upper Sco Association As* 16 12 -23.4           ~ 1586 1
14 NAME Upper Sco-Cen As* 16 15 -24.2           ~ 1497 1
15 HD 146254 V* 16 15 51.4951281264 -14 50 56.815488096   6.165 6.083     A0III 56 0
16 HD 154481 * 17 06 53.2246848982 -26 30 46.872050517   6.208 6.251     B8/9II 53 0
17 IRAS 17178-2600 PN? 17 20 56.1353525664 -26 03 30.577658436   14.408 13.627 12.879   F2Ve 25 0
18 HD 157864 * 17 26 55.2966016896 -25 56 36.474960120   6.38 6.43     B9.5/A0V 43 0

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