2025A&A...701A.281T


Query : 2025A&A...701A.281T

2025A&A...701A.281T - Astronomy and Astrophysics, volume 701A281 (2025/9-1)

Observation of new interstellar clouds in the Libra constellation inside the Local Bubble.

TOTH L.V., SLIZ-BALOGH J., MADAI A., SARI P. and HORVATH G.

Abstract (from CDS):

Context. The structure of the interstellar medium of our immediate Galactic environment has typically been studied by extinction, line emission, and absorption measurements. Interstellar clouds with moderate extinction (0.3 < AG < 1), however, may also appear as reflection nebulae in scattered light. Nearby translucent clouds may be detected by their cloud shine even inside the Local Bubble.
Aims. We explore a so far less studied area at high Galactic latitude in a search for translucent clouds inside the Local Bubble.
Methods. We mapped the sky in the visible spectral range on 21 July 2023 on the Namibian Khomas Highland with our telescope, which has a wide field of view. Optical imaging combined with multi-wavelength data helped us to localize clouds. We used Gaia DR3 data to estimate their distances and then derived their physical parameters.
Results. We detected a pattern of elongated reflection nebulae in the Libra constellation at high Galactic latitudes (l = 332°, b = 36°). The stripes of this new interstellar cloud are roughly parallel to the Galactic plane and are associated with similar structures seen in H I 21 cm maps. We identified four cloud layers: (i) The nearest component with an extinction of AG ≤ 0.2 is closer than 50 pc. (ii) The second component with an extinction of AG 0.5 has an estimated distance of 60 pc. (iii) The third component lies at 75 pc with a similar extinction. (iv) The fourth component with an extinction of AG> 1.5 and an estimated distance of 135 pc may correspond to the wall of the Local Bubble (or Local Chimney), while the former components are inside of this wall. We named these clouds the Zebra nebula system because they have strong stripes. The cloud with the highest extinction in the centre of the region we studied is called the Zebra1 nebula. The size of this interstellar cloud is 6.5 pc × 1.6 pc, and it consists of mostly neutral atomic hydrogen, but small dense parts of the cloud may be molecular. Its total mass is 70M⊙ × (d/[60] pc)2. The Zebra1 nebula is surrounded by other less opaque clouds with similar distances. They are all located inside the Local Bubble.
Conclusions. Wide-field optical imaging is capable of locating nearby high-latitude interstellar clouds. Apparently, there are still clouds to discover inside the Local Bubble (or Local Chimney).

Abstract Copyright: © The Authors 2025

Journal keyword(s): catalogs - surveys - ISM: bubbles - ISM: clouds - ISM: molecules

Simbad objects: 31

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Number of rows : 31
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 NAME LIC Cld 04 41 +31.           ~ 317 0
2 NAME NGP reg 12 51 26.275 +27 07 41.70           ~ 1274 0
3 Gaia DR3 6195375361091393408 * 13 35 03.7280219914 -22 31 52.376821596           ~ 1 0
4 DIR 316+39 IR 13 37 43 -24 24.6           ~ 3 0
5 Gaia DR3 6301365464510362368 * 14 12 00.2758580859 -14 11 50.759383484           ~ 1 0
6 TYC 6156-462-1 * 14 30 37.7518300896 -17 04 37.033038912   12.11 11.13     ~ 2 0
7 Gaia DR3 6286027964497961344 * 14 30 43.6503542431 -17 16 41.847763587           ~ 1 0
8 Gaia DR3 6286431210387704320 * 14 32 13.5441731734 -16 07 48.459715897           ~ 2 0
9 HD 128235 PM* 14 36 18.6874153512 -20 12 21.377005992   10.81 10.04     G8V 8 0
10 Gaia DR3 6280160901732789888 PM* 14 36 55.8953956962 -20 16 37.517839508           ~ 2 0
11 Gaia DR3 6286910872334996736 * 14 37 36.3555034302 -15 22 22.787576634           ~ 1 0
12 Gaia DR3 6310768247433232000 * 14 42 01.9407965818 -14 58 51.710195095           ~ 1 0
13 * alf02 Lib SB* 14 50 52.71309 -16 02 30.3955 2.99 2.90 2.75 2.61 2.57 kA2hA5mA4IV-V 231 0
14 UCAC2 25325519 PM* 14 59 06.0104297808 -17 26 48.813460692   13.42 12.08 11.72 10.46 ~ 6 0
15 Gaia DR3 6306885489622761472 * 15 03 39.7863043845 -15 55 21.952470336           ~ 1 0
16 PM J15076-1948 PM* 15 07 37.2207410856 -19 48 20.203407324   13.60 12.21 11.736 10.46 ~ 10 0
17 LDN 1780 DNe 15 39.7 -07 10           ~ 82 0
18 LDN 1778 DNe 15 39.9 -07 10           ~ 18 0
19 Gaia DR3 4396855052816597504 * 15 40 25.1789724735 -07 21 10.427276691           ~ 1 0
20 Gaia DR3 4397273833608878208 PM* 15 43 17.8237912265 -06 48 44.967404903           ~ 2 0
21 Gaia DR3 4397316435383673728 * 15 45 40.5932393613 -06 25 03.958158644           ~ 1 0
22 [DB2002b] G6.56+38.13 MoC 15 50.8 -01 41           ~ 12 0
23 LDN 169 DNe 15 52.6 -03 19           ~ 25 0
24 LDN 134 MoC 15 53 36.3 -04 35 26           ~ 217 0
25 LDN 183 MoC 15 54 12.2 -02 49 42           ~ 799 1
26 [DB2002b] G8.22+36.34 MoC 15 59 41.2 -01 41 25           ~ 17 0
27 [DB2002b] G11.39+36.22 MoC 16 05.8 +00 23           ~ 15 0
28 NAME Sco-Cen-Lup reg 16 20.0 -27 00           ~ 16 0
29 NAME Galactic Center reg 17 45 39.60213 -29 00 22.0000           ~ 16269 0
30 NAME Local Bubble ISM ~ ~           ~ 1059 0
31 NAME Local Chimney reg ~ ~           ~ 28 0

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