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J/A+A/540/A133    η Car emission spectrum (1700-10400Å)  (Zethson+, 2012)

η Carinae: linelist for the emission spectrum of the Weigelt blobs in the 1700 to 10400Å wavelength region. Zethson T., Johansson S., Hartman H., Gull T.R. <Astron. Astrophys. 540, A133 (2012)> =2012A&A...540A.133Z
ADC_Keywords: Stars, variable ; Spectroscopy Keywords: line: identification - circumstellar matter - stars: kinematics and dynamics - stars: individual: eta Carinae Abstract: We present line identifications in the 1700 to 10400Å region for the Weigelt blobs B and D, located 0.1" to 0.3" NNW of η Carinae. The aim of this work is to characterize the behavior of these luminous, dense gas blobs in response to the broad high-state and the short low-state of η Carinae during its 5.54-year spectroscopic period. Description: The spectra were recorded in a low state (March 1998) and an early high state (February 1999) with the Hubble Space Telescope/Space Telescope Imaging Spectrograph (HST/STIS) from 1640 to 10400Å using the 52"x0.1" aperture centered on Eta Carinae at position angle, PA=332 degrees. Extractions of the reduced spectrum including both Weigelt B and D, 0.28" in length along the slit, were used to identify the narrow, nebular emission lines, measure their wavelengths and estimate their fluxes. A linelist of 2500 lines is presented for the high and low states of the combined Weigelt blobs B and D. Objects: ---------------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------------- 10 45 03.59 -59 41 04.3 eta Car = HR 4210 ---------------------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file tablec1.dat 103 2537 Identifications of 2500 emission lines in the wavelength region 1700-10400Å from the STIS spectra of the Weigelt blobs recorded in March 1998 and February 1999
See also: J/A+A/304/415 : eta Car uvby-Hbeta phot. 1992-94 (van Genderen+, 1995) J/A+A/343/847 : eta Car Geneva Photometry (van Genderen+ 1999) J/A+A/419/215 : Sr filament emission lines near eta Car (Hartman+, 2004) J/AJ/129/2018 : RXTE scaled fluxes of eta Car (Corcoran+, 2005) J/A+A/493/1093 : BVRI light curves of eta Car (Fernandez-Lajus+, 2009) J/other/NewA/15.108 : UBVRIHa of eta Car in 2009 (Fernandez-Lajus+ 2010) J/ApJS/71/983 : UV spectrum of eta Car (Viotti+ 1989) J/ApJS/157/138 : UV spectrum of eta Car (Nielsen+, 2005) J/ApJS/163/173 : UV spectrum of eta Car in 2003.5 (Gull+, 2006) J/ApJS/168/289 : NUV spectrum of eta Car in 2003.5 (Nielsen+, 2007) J/ApJS/181/473 : Analysis of the spectrum of eta Car (Nielsen+, 2009) Byte-by-byte Description of file: tablec1.dat
Bytes Format Units Label Explanations
1- 8 F8.2 0.1nm lambdaO ? Observed wavelength (given in vacuum) (1) 9 A1 --- --- [-] 10- 11 I2 --- n_lambdaO ? Last 2 digits (wihtout decimals) for wavelength interval 12 A1 --- u_lambdaO [?] 14- 20 F7.1 --- Int ? Intensity (in relative units) 22- 40 A19 --- Line Line identification 42- 73 A32 --- Trans Transition 75- 82 F8.2 0.1nm lambdaL ? Laboratory wavelength (given in vacuum) (1) 84-103 A20 --- Com Comments (2)
Note (1): The identifications for the region 2424-2706Å are improved using the line list by Nielsen et al. (2007, Cat. J/ApJS/168/289) based on high resolution HST/STIS spectra. The identifications and laboratory wavelengths are retrieved from the Kurucz database (Kurucz, 2001, The laboratory wavelengths for parity forbidden lines are Ritz wavelengths derived from energy levels in the NIST Atomic Spectra Database (2006). Note (2): Comments used as follows: Not in 98 = The feature is not present in the 1998 observation Not in 99 = The feature is not present in the 1999 observation Lyα = Primary H Lyα pumped fluorescence transition Lyα sec. = Secondary H Lyα pumped fluorescence transition 4p-4s = A 4p-4s transition, discussed in section 5.5 Si III] = Fluorescence line pumped by Si III (Hartman & Johansson, 2000A&A...359..627H) He II = Fluorescence line pumped by He II (Hartman & Johansson, 2000A&A...359..627H) N IV] = Fluorescence line pumped by N IV] (Hartman & Johansson, 2000A&A...359..627H) rd_sh = red shoulder due to extended stellar wind is noticeable out to +400km/s bl_sh = blue shoulder due to extended stellar wind is noticeable out to -400km/s ? = the feature is weak and may not be a true emission line ?id = The identification is regarded as uncertain ?Eu = the upper level has an excitation energy >10eV, and the excitation mechanism is questionable ?wl = Plausible identification, but the radial velocity differs from the mean, -45km/s, by >15km/s
History: From electronic version of the journal
(End) Patricia Vannier [CDS] 12-Apr-2012
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

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