Zobrazeno 1 - 10
of 1 461
pro vyhledávání: '"York, Don"'
Autor:
Maria BARBU
Publikováno v:
Studia Universitatis Babeş-Bolyai. Philologia, Vol 69, Iss 2 (2024)
A(n) (Anarche)Typical Journey through New York: Don Delillo’s Cosmopolis as an American Postmodern Odyssey. Journeys made across the North American territories were often made in search of something: a better life, a further frontier space or the l
Externí odkaz:
https://doaj.org/article/7b10e8b9199545b69f207edc2fe35386
Autor:
BARBU, Maria
Publikováno v:
Studia Universitatis Babes-Bolyai, Philologia; Jun2024, Vol. 69 Issue 2, p109-124, 16p
Autor:
Surrency, Erwin C.
Publikováno v:
The American Journal of Legal History, 1969 Jul 01. 13(3), 312-314.
Externí odkaz:
https://www.jstor.org/stable/844535
Autor:
Szasz, Ferenc M.
Publikováno v:
New York History, 1969 Jul 01. 50(3), 328-330.
Externí odkaz:
https://www.jstor.org/stable/23162504
Autor:
Ak, N. Filiz, Brandt, W. N., Hall, P. B., Schneider, D. P., Trump, J. R., Anderson, S. F., Hamann, F., Myers, Adam D., Paris, I., Petitjean, P., Ross, Nicholas P., Shen, Yue, York, Don
We consider how the profile and multi-year variability properties of a large sample of C IV Broad Absorption Line (BAL) troughs change when BALs from Si IV and/or Al III are present at corresponding velocities, indicating that the line-of-sight inter
Externí odkaz:
http://arxiv.org/abs/1407.2250
Autor:
Ak, N. Filiz, Brandt, W. N., Hall, P. B., Schneider, D. P., Anderson, S. F., Hamann, F., Lundgren, B. F., Myers, Adam D., Paris, I., Petitjean, P., Ross, Nicholas P., Shen, Yue, York, Don
We present a detailed investigation of the variability of 428 C IV and 235 Si IV Broad Absorption Line (BAL) troughs identified in multi-epoch observations of 291 quasars by the Sloan Digital Sky Survey-I/II/III. These observations primarily sample r
Externí odkaz:
http://arxiv.org/abs/1309.5364
Autor:
Roy, Rupak, Sutaria, Firoza, Bose, Subhash, Johnson, Sean, Dwarkadas, Vikram, York, Brian, Kumar, Brijesh, Kumar, Brajesh, Bhatt, Vijay K., Chakraborti, Sayan, York, Don, Ritchey, Adam, Saurage, Gabrielle, Kaiser, Mary Beth
Supernova 2012A was discovered on 7.39UT, January, 2012 in the nearby galaxy NGC 3239 at an unfiltered magnitude of 14.6 and classified spectroscopically as a Type IIP event. Here, we present the optical photometric and spectroscopic follow-up of the
Externí odkaz:
http://arxiv.org/abs/1304.2457
Autor:
Eisenstein, Daniel J., Hogg, David W., Fukugita, Masataka, Nakamura, Osamu, Bernardi, Mariangela, Finkbeiner, Douglas P., Schlegel, David J., Brinkmann, J., Connolly, Andrew J., Csabai, Istvan, Gunn, James E., Ivezic, Zeljko, Lamb, Don Q., Loveday, Jon, Munn, Jeffrey A., Nichol, Robert C., Schneider, Donald P., Strauss, Michael A., Szalay, Alex, York, Don G.
Publikováno v:
Astrophys.J. 585 (2003) 694-713
We combine Sloan Digital Sky Survey spectra of 22,000 luminous, red, bulge-dominated galaxies to get high S/N average spectra in the rest-frame optical and ultraviolet (2600A to 7000A). The average spectra of these massive, quiescent galaxies are ear
Externí odkaz:
http://arxiv.org/abs/astro-ph/0212087
Autor:
Kauffmann, Guinevere, Heckman, Timothy M., White, Simon D. M., Charlot, Stephane, Tremonti, Christy, Peng, Eric W., Seibert, Mark, Brinkmann, Jon, Nichol, Robert C., SubbaRao, Mark, York, Don
Publikováno v:
Mon.Not.Roy.Astron.Soc.341:54,2003
We study the relations between stellar mass, star formation history, size and internal structure for a complete sample of 122,808 galaxies drawn from the Sloan Digital Sky Survey. We show that low-redshift galaxies divide into two distinct families a
Externí odkaz:
http://arxiv.org/abs/astro-ph/0205070
Autor:
Kauffmann, Guinevere, Heckman, Timothy M., White, Simon D. M., Charlot, Stephane, Tremonti, Christy, Brinchmann, Jarle, Bruzual, Gustavo, Peng, Eric W., Seibert, Mark, Bernardi, Mariangela, Blanton, Michael, Brinkmann, Jon, Castander, Francisco, Csabai, Istvan, Fukugita, Masataka, Ivezic, Zeljko, Munn, Jeffrey, Nichol, Robert, Padmanabhan, Nikhil, Thakar, Anniruddha, Weinberg, David, York, Don
Publikováno v:
Mon.Not.Roy.Astron.Soc.341:33,2003
We develop a new method to constrain the star formation histories, dust attenuation and stellar masses of galaxies. It is based on two stellar absorption line indices, the 4000 Angstrom break strength and the Balmer absorption line index Hdelta_A. To
Externí odkaz:
http://arxiv.org/abs/astro-ph/0204055