2008MNRAS.391.1107L

Query : 2008MNRAS.391.1107L

2008MNRAS.391.1107L - Mon. Not. R. Astron. Soc., 391, 1107-1116 (2008/December-2)

Integral field spectroscopy of HH 262: the spectral atlas.

LOPEZ R., GARCIA-LORENZO B., SANCHEZ S.F., GOMEZ G., ESTALELLA R. and RIERA A.

Abstract (from CDS):

HH 262 is a group of emitting knots displaying an `hour-glass' morphology in the Hα and [Sii] lines, located 3.5 arcmin to the north-east of the young stellar object L1551-IRS5, in Taurus. We present new results of the kinematics and physical conditions of HH 262 based on Integral Field Spectroscopy covering a field of ∼1.5x3 arcmin2, which includes all the bright knots in HH 262. These data show complex kinematics and significant variations in physical conditions over the mapped region of HH 262 on a spatial scale of ≤3 arcsec. A new result derived from the Integral Field Spectroscopy data is the weakness of the [Nii] emission (below detection limit in most of the mapped region of HH 262), including the brightest central knots. Our data reinforce the association of HH 262 with the redshifted lobe of the evolved molecular outflow L1551-IRS5. The interaction of this outflow with a younger one, powered by L1551 NE, around the position of HH 262 could give rise to the complex morphology and kinematics of HH 262.

Abstract Copyright: © 2008 The Authors. Journal compilation © 2008 RAS

Journal keyword(s): ISM: individual: HH 262 - ISM: individual: L1551-IRS5 - ISM: individual: L1551 NE - ISM: jets and outflows

CDS comments: In ref. list Garnavich + 1992 is 1992RMxAA.24.99G instead of 1992A&A.24.99G

Simbad objects: 36

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Number of rows : 36
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 HH 258 HH 04 31 04.791 +18 03 32.00           ~ 9 0
2 HH 28 HH 04 31 06.8 +18 03 28           ~ 94 0
3 HH 265 HH 04 31 14.965 +18 11 59.32           ~ 11 0
4 HH 102 RNe 04 31 19.2 +18 07 21           ~ 64 0
5 HH 29 HH 04 31 26.9 +18 06 39           ~ 110 0
6 LDN 1551 DNe 04 31 30.0 +18 12 30           ~ 823 1
7 RAFGL 5123 Y*O 04 31 34.07736 +18 08 04.9020           K3V/M3III 900 0
8 EM* LkHA 358 TT* 04 31 36.1433863008 +18 13 43.204853460     19.0     M0.9 97 0
9 V* V1213 Tau Or* 04 31 37.5055489536 +18 12 24.383952396           K7 605 0
10 V* HL Tau Or* 04 31 38.5107609312 +18 13 57.859747968   15.89 14.49 14.39   K5 1546 0
11 IRAS 04287+1807 mul 04 31 38.8 +18 13 57           ~ 797 0
12 V* XZ Tau Or* 04 31 40.0868968022 +18 13 56.642439056     10.40 13.12   M2e+M2e 466 2
13 2MASS J04314444+1808315 Y*O 04 31 44.44680 +18 08 31.5384           ~ 173 0
14 HH 266 HH 04 31 52.284 +18 16 49.81           ~ 9 0
15 [GH90b] 9 PoC 04 31 58.9 +18 12 07           ~ 7 0
16 [GNG92] 22 PoC 04 31 59.7 +18 10 30           ~ 3 0
17 [GNG92] 26 PoC 04 32 00.0 +18 11 17           ~ 2 0
18 JCMTSF J043200.6+181138 PoC 04 32 00.1 +18 11 34           ~ 7 0
19 [GNG92] 19 PoC 04 32 00.5 +18 12 05           ~ 4 0
20 [GH90b] 10 PoC 04 32 00.7 +18 11 24           ~ 4 0
21 [GNG92] 20 PoC 04 32 00.9 +18 11 53           ~ 3 0
22 HH 262 HH 04 32 01.082 +18 11 24.22           ~ 14 0
23 [GH90b] 10E PoC 04 32 01.1 +18 11 24           ~ 5 0
24 [GNG92] 18 PoC 04 32 01.1 +18 12 35           ~ 4 0
25 HH 262E HH 04 32 10 +18 12.3           ~ 3 0
26 HH 123 HH 04 34 49.6 -14 13 08           ~ 11 1
27 NAME Taurus Complex SFR 04 41.0 +25 52           ~ 4971 0
28 HH 126B HH 05 35 26.8 -06 22 46           ~ 8 0
29 HH 34 HH 05 35 31.30 -06 28 43.0     16     ~ 493 2
30 HH 49 HH 11 06 00.05 -77 33 36.0           ~ 34 0
31 2MASS J21450823+4733056 Y*? 21 45 08.23 +47 33 05.6           ~ 22 0
32 [GH90b] 9W PoC ~ ~           ~ 1 0
33 HH 111L HH ~ ~           ~ 18 0
34 [GNG92] 21 PoC ~ ~           ~ 4 0
35 [GH90b] 9E PoC ~ ~           ~ 1 0
36 [GH90b] 9N PoC ~ ~           ~ 1 0

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