Results 71 to 80 of about 695,772 (397)

THE CANADA-FRANCE REDSHIFT SURVEY IX: HST Imaging of High-Redshift Field Galaxies

, 1995
HST B and I images are presented of 32 CFRS galaxies with secure redshifts in the range 0.5 < z < 1.2. These galaxies exhibit the same range of morphological types as seen locally, i.e., ellipticals, spirals and irregulars.
Crampton, David, Fevre, O. Le, Hammer, F., Lilly, S. J., Schade, D. J., Tresse, L.   +5 more
core   +2 more sources

Triazine‐Trione Thermosets with High Processability for Scaffold Applications in Bone Tissue Engineering

Advanced Healthcare Materials, EarlyView.
Novel photo‐clickable triazine‐trione thermosets can be shaped and cured under mild conditions, including room and physiological temperatures. These materials are biocompatible and support osteogenic differentiation of bone marrow–derived mesenchymal stem cells on their surface.
Åshild Johansen, Shuntaro Yamada, Daniel J. Hutchinson, Mohammed A. Yassin, Samih Mohamed‐Ahmed, Cecilie Gjerde, Michael Malkoch, Kamal Mustafa   +7 more
wiley   +1 more source

Modeling the Radial Color Profile of M31

Open Astronomy, 2003
We present a preliminary study of a fragment of the radial color profile of the spiral galaxy M 31 in terms of 2-D model accounting for internal extinction in the disk. The two stellar population disk model was assumed.
Semionov D., Stonkutė R., Vansevičius V.   +2 more
doaj   +1 more source

Predictions and Outcomes for the Dynamics of Rotating Galaxies

Galaxies, 2020
A review is given of a priori predictions made for the dynamics of rotating galaxies. One theory—MOND—has had many predictions corroborated by subsequent observations.
Stacy McGaugh
doaj   +1 more source

Galaxy formation [PDF]

Symposium - International Astronomical Union, 1987
Theories of galaxy formation via hierarchical clustering of cold dark matter and by fragmentation of gaseous pancakes or shells are reviewed and compared. Dissipative processes are crucial to all theories of galaxy formation, and are discussed in terms of a simple model involving multiple cloud interactions.
openaire   +1 more source

Bar fraction in lenticular galaxies: dependence on luminosity and environment

, 2010
We present a study of bars in lenticular galaxies based on a sample of 371 galaxies from the SDSS-DR 7 and 2MASS in optical and near-infrared bands, respectively.
Abadi, Abazajian, Aguerri, Aguerri, Aguerri, Aguerri, Aguerri, Ajit K. Kembhavi, Andersen, Athanassoula, Athanassoula, Barazza, Barazza, Barr, Barway, Barway, Bekki, Boselli, Bournaud, Bureau, Combes, De Vaucouleurs, Debattista, Debattista, Elmegreen, Erwin, Eskridge, Fukugita, Gadotti, Gadotti, Ho, Hubble, Hunt, Jogee, Knapen, Kniazev, Kormendy, Laurikainen, Lisker, Marinova, Marinova, McIntosh, Mendez-Abreu, Menendez-Delmestre, Nair, Nilson, Pfenniger, Prieto, Regan, Sakamoto, Sellwood, Sheth, Sheth, Sudhanshu Barway, Tago, Thompson, Van Den Bergh, Weinzirl, Whyte, Yogesh Wadadekar   +59 more
core   +1 more source

From Spitzer Galaxy Photometry to Tully-Fisher Distances [PDF]

, 2014
This paper involves a data release of the observational campaign: Cosmicflows with Spitzer (CFS). Surface photometry of the 1270 galaxies constituting the survey is presented.
Courtois, H. M., Jarrett, T. H., Neill, J. D., Shaya, E. J., Sorce, J. G., Tully, R. B.   +5 more
core   +4 more sources

End‐to‐End Sensing Systems for Breast Cancer: From Wearables for Early Detection to Lab‐Based Diagnosis Chips

Advanced Materials Technologies, EarlyView.
This review explores advances in wearable and lab‐on‐chip technologies for breast cancer detection. Covering tactile, thermal, ultrasound, microwave, electrical impedance tomography, electrochemical, microelectromechanical, and optical systems, it highlights innovations in flexible electronics, nanomaterials, and machine learning.
Neshika Wijewardhane, Lyn I. Jones, Richard M. Martin, Helen Winter, Faezeh Arab Hassani   +4 more
wiley   +1 more source

What Does Clustering Tell Us About the Buildup of the Red Sequence?

, 2009
We analyze the clustering of red and blue galaxies from four samples spanning a redshift range of 0 ...
Abbas, Andrew R. Wetzel, Bell, Berlind, Berlind, Blanton, Blanton, Brown, Coil, Conroy, Conroy, Driver, Dunkley, Hamilton, Hansen, Hopkins, Hopkins, Jannuzi, Jeremy L. Tinker, Kaiser, Kang, Kang, Kochanek, Koester, Kravtsov, Kriek, Kriek, Labbé, Lin, Maller, Maller, Marchesini, Marín, McCracken, Moster, Nagai, Negroponte, Noeske, Papovich, Quadri, Quadri, Scoccimarro, Somerville, Strateva, Tinker, Tinker, Tinker, Tinker, Tinker, Tinker, Tinker, White, White, Williams, Willmer, Yang, Zehavi, Zhao, Zheng, Zheng, Zheng, Zheng   +61 more
core   +2 more sources

Quantitative Morphology of Galaxies in the Hubble Deep Field [PDF]

, 1998
We measure quantitative structural parameters of galaxies in the Hubble Deep Field (HDF) on the drizzled F814W images. Our structural parameters are based on a two-component surface brightness made up of a S\'ersic profile and an exponential profile.
Abraham R. G., Cole S., de Vaucouleurs G., de Vaucouleurs G., de Vaucouleurs G., Doi M., Ellis R. S., Francine R. Marleau, Kauffmann G., Luc Simard, Michard R., Navarro J. F., Patterson F. S., Steinmetz M.   +13 more
core   +2 more sources