Results 1 to 10 of about 9,614 (265)

The Astrophysics of Emission-Line Stars [PDF]

open access: yesAstrophysics and Space Science Library, 2007
Tomokazu Kogure, Kam-Ching Leung
exaly   +2 more sources

A Study of Emission Lines in Carbon Stars

open access: yesThe Astrophysical Journal
Carbon stars are chemically peculiar stars with high carbon abundance, showing strong carbon molecule bands and rare emission lines in their spectra. This paper explores the stellar activity of carbon stars by identifying emission line features in their ...
Lichan Zhou   +5 more
doaj   +2 more sources

Modelling emission lines in star-forming galaxies [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2021
ABSTRACT We present a new model to compute the luminosity of emission lines in star-forming galaxies and apply this in the semi-analytical galaxy formation code galform. The model combines a pre-computed grid of H II region models with an empirical determination of how the properties of H II regions depend on the macroscopic properties ...
C M Baugh   +3 more
openaire   +3 more sources

The Weak Emission Line Stars [PDF]

open access: yesSymposium - International Astronomical Union, 2003
In this paper, we study the evolution of the weak emission line central stars of planetary nebula (WELS), which are similar to the H-deficient Wolf-Rayet central stars except for systematically weaker emission lines. Our attempts at finding an evolutionary sequence for the WELS similar to what was established for Wolf-Rayet central stars, were ...
Jeffrey Fogel   +2 more
openaire   +1 more source

Infrared Lines in Peculiar Emission-Line Stars [PDF]

open access: yesSymposium - International Astronomical Union, 1976
An image-tube Cassegrain spectrograph, equipped with an S-1 photocathode enabled us to obtain infrared spectra of peculiar emission-line objects, as V 1016 Cyg, HBV 475, HD 51585, HD 45677, XX Oph and CI Cyg. Many of these objects display emission lines of H I, He I, He II, O I, N I, Ca II [S II] [S III], [Fe II].
Y. Andrillat, L. Houziaux
openaire   +1 more source

A photometric catalogue of southern emission-line stars [PDF]

open access: yesAstronomy & Astrophysics, 2001
We present a catalogue of previously unpublished optical and infrared photometry for a sample of 162 emission-line objects and shell stars visible from the southern hemisphere. The data were obtained between 1978 and 1997 in the Walraven (WULBV), Johnson/Cousins (UBV(RI)_c) and ESO and SAAO near-infrared (JHKLM) photometric systems.
de Winter, D.   +7 more
openaire   +2 more sources

The atypical emission-line star Hen 3-209 [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2006
6p, 5 fig, accepted for publication in MNRAS (www.blackwell-synergy.com)
Nazé, Yaël   +5 more
openaire   +3 more sources

Rapid Variability of H α Emission Line in Be Stars [PDF]

open access: yesSymposium - International Astronomical Union, 1994
We have initiated an observational campaign on some bright Be stars in order to investigate the rapid variability in emission lines using a Fabry-Perot spectrometer(λ/δλ = 104; FSR = 21.3Å) at the Nasmyth focus of the 1.22 m JRO telescope at Hyderabad, India. The PMT dark counts were 1 – 2sec-1. Here we report our first observations on four stars.
B. G. Anandarao   +3 more
openaire   +1 more source

HYDROGEN LINES IN B-e STARS ENVELOPES

open access: yesOdessa Astronomical Publications, 2017
The investigation of Balmer Hα and Hb line profiles for 28 Be and Be-shell stars have been carried out. The emission profiles of stars were obtained by subtracting from “A Be star atlas” photospheric line profiles which were computed from Kurucz models ...
S. N. Udovichenko, E. I. Konchagina
doaj   +1 more source

UV line emission of symbiotic stars [PDF]

open access: yesInternational Astronomical Union Colloquium, 1982
AbstractGeneral characteristics of emission line spectra from symbiotic stars are outlined. Data from some special line ratios in the 1000 Å - 3000 Å range, and others connecting the visual and the far UV lines are presented, and their application to symbiotic stars is discussed.
openaire   +1 more source

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