The Evolution of Balmer Absorption-Line Strengths in E/S0 Galaxies from [FORMULA][F]z=0[/F][/FORMULA] to [FORMULA][F]z=0.83[/F][/FORMULA]

2001 ◽  
Vol 552 (1) ◽  
pp. L17-L21 ◽  
Author(s):  
Daniel D. Kelson ◽  
Garth D. Illingworth ◽  
Marijn Franx ◽  
Pieter G. van Dokkum
Keyword(s):  
Absorption Line ◽  
S0 Galaxies ◽  
Line Strengths

scholarly journals S0 Galaxy Line Strengths and Gradients

1996 ◽  
Vol 171 ◽  
pp. 374-374
Author(s):  
David Fisher ◽  
Marijn Franx ◽  
Garth Illingworth
Keyword(s):  
Stellar Populations ◽  
Elliptical Galaxies ◽  
S0 Galaxies ◽  
Line Strengths

Line strengths and their gradients in Mg, Fe, and Hβ have been determined for a sample of 20 S0 galaxies in order to study the stellar populations of their bulges and disks and to investigate their relationship to elliptical galaxies. The data were obtained with the Lick Observatory 3m telescope in the long-slit mode over the region 4215–5615 Å with resolution 3.1 Å.

Line Strengths and Line-Strength Gradients in S0 Galaxies

1996 ◽  
Vol 459 ◽  
pp. 110 ◽  
Author(s):  
David Fisher ◽  
Marijn Franx ◽  
Garth Illingworth
Keyword(s):  
Line Strength ◽  
S0 Galaxies ◽  
Line Strengths

scholarly journals Absorption-line strengths of 18 late-type spiral galaxies observed with SAURON

2007 ◽  
Vol 380 (2) ◽  
pp. 506-540 ◽  
Author(s):  
Katia Ganda ◽  
Reynier F. Peletier ◽  
Richard M. McDermid ◽  
Jesús Falcón-Barroso ◽  
P. T. De Zeeuw ◽  
...  
Keyword(s):  
Absorption Line ◽  
Spiral Galaxies ◽  
Late Type ◽  
Line Strengths

scholarly journals Gradients of Absorption‐Line Strengths in Elliptical Galaxies

1999 ◽  
Vol 527 (2) ◽  
pp. 573-599 ◽  
Author(s):  
Chiaki Kobayashi ◽  
Nobuo Arimoto
Keyword(s):  
Absorption Line ◽  
Elliptical Galaxies ◽  
Line Strengths

scholarly journals The Strongly Polarized P Cygni Star with Infrared Excess CPD −52° 9243

1982 ◽  
Vol 98 ◽  
pp. 101-102
Author(s):  
J. P. Swings
Keyword(s):  
Absorption Line ◽  
Spectral Type ◽  
Visible Spectrum ◽  
Infrared Excess ◽  
Strong Polarization ◽  
Astronomy And Astrophysics ◽  
Line Strengths

The visible spectrum of the point-like source with infrared excess CPD-52°9243 is identified; emission and absorption line strengths are given together with various ion velocities of P Cygni profiles; a strong polarization is detected: P ≃ 5 %, θ ≃ 36°. From stellar and interstellar features, a spectral type around B8Ia and a distance of about 3.1 kpcs are derived.A detailed publication is presently in press in Astronomy and Astrophysics.

Absorption line strengths of 15NH3 in the near infrared spectral region

2010 ◽  
Vol 102 (2) ◽  
pp. 293-301 ◽  
Author(s):  
B. Lins ◽  
F. Pflaum ◽  
R. Engelbrecht ◽  
B. Schmauss
Keyword(s):  
Absorption Line ◽  
Spectral Region ◽  
Near Infrared ◽  
Infrared Spectral Region ◽  
Infrared Spectral ◽  
Line Strengths
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