Zobrazeno 1 - 10
of 158
pro vyhledávání: '"Moe, Maxwell"'
Autor:
Belloni, Diogo, Zorotovic, Monica, Schreiber, Matthias R., Parsons, Steven G., Moe, Maxwell, Garbutt, James A.
Publikováno v:
A&A 686, A61 (2024)
In this first in a series of papers related to long-period post-common-envelope (CE) binaries, we investigated whether extra energy is required or not to explain the currently known post-CE binaries with sufficiently long orbital periods consisting o
Externí odkaz:
http://arxiv.org/abs/2401.07692
Context. Recent observations of close detached eclipsing M and K dwarf binaries have provided substantial support for magnetic saturation when stars rotate sufficiently fast, leading to a magnetic braking (MB) torque proportional to the spin of the s
Externí odkaz:
http://arxiv.org/abs/2311.04309
Binary stars evolve into chemically-peculiar objects and are a major driver of the Galactic enrichment of heavy elements. During their evolution they undergo interactions, including tides, that circularize orbits and synchronize stellar spins, impact
Externí odkaz:
http://arxiv.org/abs/2307.02678
Autor:
Shen, Yue, Grier, Catherine J., Horne, Keith, Stone, Zachary, Li, Jennifer I., Yang, Qian, Homayouni, Yasaman, Trump, Jonathan R., Anderson, Scott F., Brandt, W. N., Hall, Patrick B., Ho, Luis C., Jiang, Linhua, Petitjean, Patrick, Schneider, Donald P., Tao, Charling, Donnan, Fergus. R., AlSayyad, Yusra, Bershady, Matthew A., Blanton, Michael R., Bizyaev, Dmitry, Bundy, Kevin, Chen, Yuguang, Davis, Megan C., Dawson, Kyle, Fan, Xiaohui, Greene, Jenny E., Groller, Hannes, Guo, Yucheng, Ibarra-Medel, Hector, Jiang, Yuanzhe, Keenan, Ryan P., Kollmeier, Juna A., Lejoly, Cassandra, Li, Zefeng, de la Macorra, Axel, Moe, Maxwell, Nie, Jundan, Rossi, Graziano, Smith, Paul S., Tee, Wei Leong, Weijmans, Anne-Marie, Xu, Jiachuan, Yue, Minghao, Zhou, Xu, Zhou, Zhimin, Zou, Hu
We present the final data from the Sloan Digital Sky Survey Reverberation Mapping (SDSS-RM) project, a precursor to the SDSS-V Black Hole Mapper Reverberation Mapping program. This data set includes 11-year photometric and 7-year spectroscopic light
Externí odkaz:
http://arxiv.org/abs/2305.01014
Autor:
Murphy, Simon J, Moe, Maxwell, Kurtz, Donald W, Bedding, Timothy R, Shibahashi, Hiromoto, Boffin, Henri M J
The orbital parameters of binaries at intermediate periods (10(2)-10(3) d) are difficult to measure with conventional methods and are very incomplete. We have undertaken a new survey, applying our pulsation timing method to Kepler light curves of 222
Externí odkaz:
http://hdl.handle.net/10150/627133
http://arizona.openrepository.com/arizona/handle/10150/627133
http://arizona.openrepository.com/arizona/handle/10150/627133
Autor:
Badenes, Carles, Mazzola, Christine, Thompson, Todd A., Covey, Kevin, Freeman, Peter E., Walker, Matthew G., Moe, Maxwell, Troup, Nicholas, Nidever, David, Prieto, Carlos Allende, Andrews, Brett, Barbá, Rodolfo H., Beers, Timothy C., Bovy, Jo, Carlberg, Joleen K., Lee, Nathan De, Johnson, Jennifer, Lewis, Hannah, Majewski, Steven R., Pinsonneault, Marc, Sobeck, Jennifer, Stassun, Keivan G., Stringfellow, Guy S., Zasowski, Gail
We use the multi-epoch radial velocities acquired by the Apache Point Observatory Galactic Evolution Experiment (APOGEE) survey to perform a large-scale statistical study of stellar multiplicity for field stars in the Milky Way, spanning the evolutio
Externí odkaz:
http://hdl.handle.net/10150/627094
http://arizona.openrepository.com/arizona/handle/10150/627094
http://arizona.openrepository.com/arizona/handle/10150/627094
Autor:
Moe, Maxwell, Kratter, Kaitlin M.
Solar-type binaries with short orbital periods (P-close equivalent to 1-10. days; a less than or similar to 0.1. au) cannot form directly via fragmentation of molecular clouds or protostellar disks, yet their component masses are highly correlated, s
Externí odkaz:
http://hdl.handle.net/10150/627100
http://arizona.openrepository.com/arizona/handle/10150/627100
http://arizona.openrepository.com/arizona/handle/10150/627100
Autor:
Kostov, Veselin B., Borkovits, Tamas, Rappaport, Saul A., Powell, Brian P., Pal, Andras, Jacobs, Thomas L., Gagliano, Robert, Kristiansen, Martti H., LaCourse, Daryll M., Moe, Maxwell, Omohundro, Mark, Schmitt, Allan R., Schwengeler, Hans M., Terentev, Ivan A., Vanderburg, Andrew
We present the discovery of a new highly compact quadruple star system, TIC 219006972, consisting of two eclipsing binary stars with orbital periods of 8.3 days and 13.7 days, and an outer orbital period of only 168 days. This period is a full factor
Externí odkaz:
http://arxiv.org/abs/2303.14275
Autor:
Moe, Maxwell, Di Stefano, Rosanne
We compile observations of early-type binaries identified via spectroscopy, eclipses, long-baseline interferometry, adaptive optics, common proper motion, etc. Each observational technique is sensitive to companions across a narrow parameter space of
Externí odkaz:
http://hdl.handle.net/10150/624451
http://arizona.openrepository.com/arizona/handle/10150/624451
http://arizona.openrepository.com/arizona/handle/10150/624451
Autor:
Evans, Nancy Remage, Engle, Scott, Pillitteri, Ignazio, Guinan, Edward, Günther, H. Moritz, Wolk, Scott, Neilson, Hilding, Marengo, Massimo, Matthews, Lynn D., Moschou, Sofia, Drake, Jeremy J., Winston, Elaine M., Moe, Maxwell, Kervella, Pierre, Breuval, Louise
X-ray observations have been made of a sample of 20 classical Cepheids, including two new observations (Polaris and {\it l} Car) reported here. The occurrence of X-ray flux around the pulsation cycle is discussed. Three Cepheids are detected ($\delta
Externí odkaz:
http://arxiv.org/abs/2205.07967