2014A&A...569A..92V


C.D.S. - SIMBAD4 rel 1.7 - 2020.07.12CEST12:09:16

2014A&A...569A..92V - Astronomy and Astrophysics, volume 569A, 92-92 (2014/9-1)

From the ashes: JVLA observations of water fountain nebula candidates show the rebirth of IRAS 18455+0448.

VLEMMINGS W.H.T., AMIRI N., VAN LANGEVELDE H.J. and TAFOYA D.

Abstract (from CDS):

The class of water fountain nebulae is thought to represent the stage of the earliest onset of collimated bipolar outflows during the post-asymptotic giant branch phase. They thus play a crucial role in the study of the formation of bipolar planetary nebulae (PNe). To date, 14 water fountain nebulae have been identified. The identification of more sources in this unique stage of stellar evolution will enable us to study the origin of bipolar PNe morphologies in more detail. Water fountain candidates can be identified based on the often double peaked 22GHz H2O maser spectrum with a large separation between the maser peaks (often >100km/s). However, even a fast bipolar outflow will only have a moderate velocity extent in its maser spectrum when located close to the plane of the sky. In this project we aim to enhance the water fountain sample by identifying objects whose jets are aligned close to the plane of the sky. We present the results of seven sources observed with the Jansky Very Large Array (JVLA) that were identified as water fountain candidates in an Effelsberg 100m telescope survey of 74 AGB and early post-AGB stars. We find that our sample of water fountain candidates displays strong variability in their 22GHz H2O maser spectra. The JVLA observations show an extended bipolar H2O maser outflow for one source, the OH/IR star IRAS 18455+0448. This source was previously classified as a dying OH/IR star based on the exponential decrease of its 1612MHz OH maser and the lack of H2O masers. We therefore also re-observed the 1612, 1665, and 1667MHz OH masers. We confirm that the 1612MHz masers have not reappeared and find that the1665/1667MHz masers have decreased in strength by several orders of magnitude during the last decade. The JVLA observations also reveal a striking asymmetry in the red-shifted maser emission of IRAS 19422+3506. The OH/IR star IRAS 18455+0448 is confirmed to be a new addition to the class of water fountain nebulae. Its kinematic age is ∼70yr, but could be lower, depending on the distance and inclination. Previous observations indicate, with significant uncertainty, that IRAS 18455+0448 has a surprisingly low mass compared to available estimates for other water fountain nebulae. The available historical OH maser observations make IRAS 18455+0448 unique for the study of water fountain nebulae and the launch of post-AGB bipolar outflows. The other candidate sources appear high mass-loss OH/IR stars with partly radially beamed H2O masers.

Abstract Copyright:

Journal keyword(s): stars: AGB and post-AGB - masers

Simbad objects: 12

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Number of rows : 12

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2020
#notes
1 IRAS 18455+0448 AB* 18 48 02.3024045147 +04 51 30.472551645           ~ 20 0
2 NVSS J185146+003532 Rad 18 51 46.72295 +00 35 32.3649           ~ 54 1
3 RAFGL 2290 OH* 18 58 30.0947842133 +06 42 57.698061173           ~ 120 0
4 OH 42.3 -0.1 OH* 19 09 07.4662208672 +08 16 22.702583816       16.16   ~ 79 0
5 IRAS 19069+0916 Y*? 19 09 19.263 +09 21 11.51           ~ 14 0
6 IRAS 19112+0819 IR 19 13 37.32 +08 24 52.4           ~ 6 0
7 IRAS 19186+0315 * 19 21 11.7099573257 +03 20 57.757377912           ~ 15 0
8 GB6 B1920+1524 Rad 19 22 34.69927882 +15 30 10.0322171           ~ 38 0
9 ICRF J192559.6+210626 QSO 19 25 59.60535560 +21 06 26.1620442           ~ 177 1
10 OH 51.8 -0.1 OH* 19 27 42.04 +16 37 24.0           ~ 37 1
11 RAFGL 2445 OH* 19 44 07.0007537378 +35 14 08.251836769           M7.5III 31 0
12 QSO B2005+40 QSO 20 07 44.9443187008 +40 29 48.601470737   18.5 19 20.3   ~ 268 1

    Equat.    Gal    SGal    Ecl

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2020.07.12-12:09:16

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