Morphology and environment of galaxies with disc breaks in the S4G and NIRS0S (vol 441, 3, 2015)

被引：0

作者：

Laine, J. ^{[1
]}

Laurikainen, E. ^{[1
,2
]}

Salo, H. ^{[1
]}

Comeron, S. ^{[1
,2
]}

Buta, R. J. ^{[3
]}

Zaritsky, D. ^{[4
]}

Athanassoula, E. ^{[5
]}

Bosma, A. ^{[5
]}

Munoz-Mateos, J-C. ^{[6
,7
]}

Gadotti, D. A. ^{[6
]}

Hinz, J. L. ^{[8
]}

Erroz-Ferrer, S. ^{[9
,10
]}

de Paz, A. Gil ^{[11
]}

Kim, T. ^{[6
,7
,12
]}

Menendez-Delmestre, K. ^{[13
]}

Mizusawa, T. ^{[7
,14
]}

Regan, M. W. ^{[15
]}

Seibert, M. ^{[16
]}

Sheth, K. ^{[7
]}

机构：

[1] Univ Oulu, Astron Div, Dept Phys, FI-90014 Oulu, Finland

[2] Univ Turku, Finnish Ctr Astron ESO FINCA, FI-21500 Piikkio, Finland

[3] Univ Alabama, Dept Phys & Astron, Tuscaloosa, AL 35487 USA

[4] Univ Arizona, Tucson, AZ 85721 USA

[5] Aix Marseille Univ, CNRS, LAM, UMR 7326, F-13388 Marseille, France

[6] European So Observ, Santiago 19, Chile

[7] Natl Radio Astron Observ NAASC, Charlottesville, VA 22903 USA

[8] Univ Arizona, MMTO, Tucson, AZ 85721 USA

[9] Inst Astrofis Canarias, E-38205 San Cristobal la Laguna, Spain

[10] Univ La Laguna, Dept Astrofis, E-38206 San Cristobal la Laguna, Spain

[11] Univ Complutense Madrid, Dept Astrofis, E-28040 Madrid, Spain

[12] Seoul Natl Univ, Dept Phys & Astron, Astron Program, Seoul 151742, South Korea

[13] Univ Fed Rio de Janeiro, Observ Valongo, BR-20080090 Rio De Janeiro, Brazil

[14] Florida Inst Technol, Melbourne, FL 32901 USA

[15] Space Telescope Sci Inst, Baltimore, MD 21218 USA

[16] Observ Carnegie Inst Washington, Pasadena, CA 91101 USA

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2016年 / 456卷 / 01期

关键词：

errata; addenda; galaxies: evolution; galaxies: formation; galaxies: interactions; galaxies: photometry; galaxies: structure;

D O I：

10.1093/mnras/stv2779

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：844 / 844

页数：1

共 34 条

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[32] MID-INFRARED GALAXY MORPHOLOGY FROM THE SPITZER SURVEY OF STELLAR STRUCTURE IN GALAXIES (S4G): THE IMPRINT OF THE DE VAUCOULEURS REVISED HUBBLE-SANDAGE CLASSIFICATION SYSTEM AT 3.6 μm [J].

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[33] RECONSTRUCTING THE STELLAR MASS DISTRIBUTIONS OF GALAXIES USING S4G IRAC 3.6 AND 4.5 μm IMAGES. II. THE CONVERSION FROM LIGHT TO MASS [J].

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[34] RECONSTRUCTING THE STELLAR MASS DISTRIBUTIONS OF GALAXIES USING S4G IRAC 3.6 AND 4.5 μm IMAGES. I. CORRECTING FOR CONTAMINATION BY POLYCYCLIC AROMATIC HYDROCARBONS, HOT DUST, AND INTERMEDIATE-AGE STARS [J].

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