The Diffuse Light Envelope of Luminous Red Galaxies
Y. Leung, Y. Zhang, B. Yanny, K. Herner, J. Annis, A. Palmese, H. Sampaio-Santos, V. Strazzullo, M. Aguena, S. Allam, S. Avila, E. Bertin, S. Bhargava, D. Brook… 展开作者
Y. Leung, Y. Zhang, B. Yanny, K. Herner, J. Annis, A. Palmese, H. Sampaio-Santos, V. Strazzullo, M. Aguena, S. Allam, S. Avila, E. Bertin, S. Bhargava, D. Brooks, D. L. Burke, A. Carnero Rosell, M. Carrasco Kind, J. Carretero, M. Costanzi, L. N. DaCosta, S. Desai, H. T. Diehl, P. Doel, T. F. Eifler, S. Everett, B. Flaugher, J. Frieman, J. García-Bellido, E. Gaztanaga, D. Gruen, R. A. Gruendl, J. Gschwend, G. Gutierrez, K. Honscheid, D. J. James, A. G. Kim, K. Kuehn, N. Kuropatkin, M. Lima, M. A. G. Maia, R. Miquel, R. L. C. Ogando, F. Paz-Chinchón, A. A. Plazas, A. K. Romer, A. Roodman, E. S. Rykoff, E. Sanchez, V. Scarpine, M. Schubnell, S. Serrano, I. Sevilla-Noarbe, M. Smith, E. Suchyta, M. E. C. Swanson, T. N. Varga
We use a stacking method to study the radial light profiles of luminous red galaxies (LRGs) at redshift $\sim 0.62$ and $\sim 0.25$, out to a radial range of 200 kpc. We do not find noticeable evolution of the profiles at the two redshifts. The LRG profiles appear to be well approximated by a single Sersic profile, although some excess light can be seen outside 60 kpc. We quantify the excess light by measuring the integrated flux and find that the excess is about 10\% -- a non-dominant but still nonnegligible component.
The nature of Cloud-9: a compact core embedded in a diffuse envelope
National Astronomical Observatories, Chinese Academy of Sciences(中国科学院国家天文台);University of Chinese Academy of Sciences(中国科学院大学);Guizhou University(贵州大学)
Broad Balmer Wings in BA Hyper/Supergiants Distorted by Diffuse Interstellar Bands: Five Examples in the 30 Doradus Region from the VLT-FLAMES Tarantula Survey
Comparative Study of Two Luminous Red Novae I. Progenitor Modeling and Dust Formation
Institut de Ciències del Cosmos (ICCUB), Universitat de Barcelona (UB)(巴塞罗那大学宇宙科学研究所);Departament de Física Quàntica i Astrofísica (FQA), Universitat de Barcelona (UB)(巴塞罗那大学量子物理与天体物理学系);Institut d’Estudis Espacials de Catalunya (IEEC)(加泰罗尼亚空间研究院);Department of Astrophysics/IMAPP, Radboud University(拉德堡德大学天体物理学/IMAPP系)