Zobrazeno 1 - 9
of 9
pro vyhledávání: '"Linder, Tyler"'
Autor:
Caddy, Robert V., Layden, Andrew C., Reichart, Daniel E., Haislip, Joshua B., Kouprianov, Vladimir V., Ivarsen, Kevin M., Moore, Justin P., LaCluyze, Aaron P., Linder, Tyler R., Nysewander, Melissa C.
Publikováno v:
PASP 134 094201 (2022)
We present time-series CCD photometry in the $BVRI$ passbands of the recently identified symbiotic nova V1835 Aquilae (NSV 11749) over an interval of 5.1 years with 7-14 day cadence, observed during its quiescence. We find slow light variations with
Externí odkaz:
http://arxiv.org/abs/2209.11251
Autor:
Satpathy, Akash, Mainzer, Amy, Masiero, Joseph R., Linder, Tyler, Cutri, Roc M., Wright, Edward L., Pittichova, Jana, Grav, Tommy, Kramer, Emily
Large potentially hazardous asteroids (PHAs) are capable of causing a global catastrophe in the event of a planetary collision. Thus, rapid assessment of such an object's physical characteristics is crucial for determining its potential risk scale. W
Externí odkaz:
http://arxiv.org/abs/2204.05412
Using data from the Sloan Digital Sky Survey Moving Object Catalog, we study color as a function of size for C-complex families in the Main Asteroid Belt to improve our understanding of space weathering of carbonaceous materials. We find two distinct
Externí odkaz:
http://arxiv.org/abs/2101.08822
Autor:
Linder, Tyler R.
Researchers have been categorizing asteroids by color for decades in an attempt to better understand asteroid composition and potential links to the meteorite population. However, only recently through large data collection surveys like the Sloan Dig
Externí odkaz:
http://pqdtopen.proquest.com/#viewpdf?dispub=10616215
Autor:
Sanchez, Juan A., Reddy, Vishnu, Thirouin, Audrey, Wright, Edward L., Linder, Tyler R., Kareta, Theodore, Sharkey, Benjamin
Main belt asteroid (6478) Gault has been dynamically linked with two overlapping asteroid families: Phocaea, dominated by S-type asteroids, and Tamara, dominated by low-albedo C-types. This object has recently become an interesting case for study, af
Externí odkaz:
http://arxiv.org/abs/1907.06643
Autor:
Hutchens, Zackary L., Barlow, Brad N., Soto, Alan Vasquez, Reichart, Dan E., Haislip, Josh B., Kouprianov, Vladimir V., Linder, Tyler R., Moore, Justin P.
CS 1246 is a hot subdwarf B star discovered in 2009 to exhibit a single, large-amplitude radial pulsation. An O-C diagram constructed from this mode revealed reflex motion due to the presence of a low-mass M dwarf, as well as a long-term trend consis
Externí odkaz:
http://arxiv.org/abs/1712.02392
Autor:
Boudreaux, Emily M., Barlow, Brad N., Fleming, Scott W., Soto, Alan Vasquez, Million, Chase, Reichart, Dan E., Haislip, Josh B., Linder, Tyler R., Moore, Justin P.
NASA's Galaxy Evolution Explorer (GALEX) provided near- and far-UV observations for approximately 77 percent of the sky over a ten-year period; however, the data reduction pipeline initially only released single NUV and FUV images to the community. T
Externí odkaz:
http://arxiv.org/abs/1708.00839
Autor:
Hutchens Zackary L., Barlow Brad N., Soto Alan Vasquez, Reichart Dan E., Haislip Josh B., Kouprianov Vladimir V., Linder Tyler R., Moore Justin P.
Publikováno v:
Open Astronomy, Vol 26, Iss 1, Pp 252-257 (2017)
CS 1246 is a hot subdwarf B star discovered in 2009 to exhibit a single, large-amplitude radial pulsation. An O-C diagram constructed from this mode revealed reflex motion due to the presence of a low-mass M dwarf, as well as a long-term trend consis
Externí odkaz:
https://doaj.org/article/88416f186f484112a5439e9fc2acb920
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