J/A+A/689/A70       [FeII] 1.644um imaging survey of 5 PNe        (Akras+, 2024)

[Fe II] 1.644um imaging survey of planetary nebulae with low-ionisation structures. Akras S., Aleman I., Goncalves R.D., Ramos-Larios G., Bouvis K. <Astron. Astrophys. 689, A70 (2024)> =2024A&A...689A..70A 2024A&A...689A..70A (SIMBAD/NED BibCode)
ADC_Keywords: Planetary nebulae; Interstellar medium ; Infrared Keywords: shock waves - ISM: atoms - ISM: jets and outflows - photon-dominated region (PDR) - infrared: general Abstract: Low-ionisation structures (LISs) are commonly found in planetary nebulae (PNe), but they are still poorly understood. The recent discovery of unforeseen molecular hydrogen gas (H2) has impacted what we think we know about these microstructures and PNe. To obtain an overall understanding of LISs, we carried out an [FeII] 1.644um imagery survey in PNe with LISs, with the aim to detect the [FeII] 1.644um emission line, a common tracer of shocks. We present the first detection of [FeII] 1.644um line directly associated with the LISs in four out of five PNe. The theoretical H I 12-4 recombination line was also computed either from the Brgamma or the Hbeta line and subtracted from the observed narrow-band line fluxes. The [FeII] 1.644um flux ranges from 1 to 40x10-15erg/cm2/s and the intensity from 2 to 90x10-5erg/s/cm2/sr. The R(Fe)=[FeII]1.644mu/Brgamma line ratio was also computed and found to range between 0.5 and 7. In particular, the [FeII] 1.644um line was detected in NGC 6543 (R(Fe)<0.15), along with the outer pairs of LISs in NGC 7009 (R(Fe)<0.25) and the jet-like LISs in IC 4634 (R(Fe)∼1) and in several LISs in NGC 6571 (2<R(Fe)<7). The low R(Fe) result for NGC 6543 is attributed to the UV radiation from the central star. In contrast, the higher values in NGC 6571 and IC 4634 are indicative of shocks. The moderate R(Fe) in NGC 7009 likely indicates the contribution of both mechanisms. Description: A near-IR (NIR) narrow-band imaging survey of PNe with LISs was carried out in 2017 (February 20, March 25, June 6 and 9, and July 2 and 3, Program ID: GN-2017A-Q-58, PI: S. Akras) in service mode, using the Near InfraRed Imager and Spectrometer on the Gemini-North Telescope at Mauna Kea in Hawaii. The narrow-band filter G0215 was used to isolate the [FeII] line centered at 1.644um, while the narrow-band H-continuum filter (G0214) at 1.570um was used to determine and finally remove any adjacent continuum emission. Narrow-band G0215 ([FeII]+HI 12-4) emission line and continuum-subtracted [FeII]+HI 12-4 emission line images of NGC6210, IC4634, NGC6543, NGC6751 and NGC7009 Objects: ------------------------------------------------------ RA (2000) DE Designation(s) ------------------------------------------------------ 21 04 10.82 -11 21 48.6 NGC 7009 = PN G037.7-34.5 17 58 33.40 +66 37 58.7 NGC 6543 = PN G096.4+29.9 19 05 55.53 -05 59 32.3 NGC 6751 = PN G029.2-05.9 16 44 29.52 +23 47 59.4 NGC 6210 = PN G043.1+37.7 17 01 33.58 -21 49 33.0 IC 4634 = PN G000.3+12.2 ------------------------------------------------------ File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file list.dat 128 12 List of fits images fits/* . 12 Individual fits images -------------------------------------------------------------------------------- Byte-by-byte Description of file: list.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 7 A7 --- Name PN name 9- 10 I2 h RAh Right Ascension (J2000) 12- 13 I2 min RAm Right Ascension (J2000) 15- 19 F5.2 s RAs Right Ascension (J2000) 20 A1 --- DE- Declination sign (J2000) 21- 22 I2 deg DEd Declination (J2000) 24- 25 I2 arcmin DEm Declination (J2000) 27- 30 F4.1 arcsec DEs Declination (J2000) 32- 36 F5.3 arcsec/pix scale Scale of the image 38- 41 I4 --- Nx Number of pixels along X-axis 43- 46 I4 --- Ny Number of pixels along Y-axis 48- 51 I4 Kibyte size Size of FITS file 53- 64 A12 --- FileName Name of FITS file, in subdirectory fits 66-128 A63 --- Title Title of the FITS file -------------------------------------------------------------------------------- Acknowledgements: Stavros Akras, stavrosakras(at)gmail.com
(End) Patricia Vannier [CDS] 29-Jul-2024
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line