Zobrazeno 1 - 10
of 26
pro vyhledávání: '"Flowers, Erin"'
Publikováno v:
Planet. Sci. J. 4 (2023) 127
Thermochemical modeling and shock-tube experiments show that shocks applied to N$_2$/CH$_4$ gas mixtures can synthesize organic molecules. Sufficiently large, hypersonic meteoroids entering the atmosphere of Saturn's moon Titan should therefore drive
Externí odkaz:
http://arxiv.org/abs/2307.10293
The Cassini-Huygens mission measured the chemical abundances of the major components of Titan's atmosphere, and analyses of the data revealed several as-yet unexplained anomalies in the methane and hydrogen profiles. We model the deceleration and abl
Externí odkaz:
http://arxiv.org/abs/2107.10336
Autor:
Gan, Tianjun, Wang, Sharon Xuesong, Teske, Johanna K., Mao, Shude, Howard, Ward S., Law, Nicholas M., Batalha, Natasha E., Vanderburg, Andrew, Dragomir, Diana, Huang, Chelsea X., Feng, Fabo, Butler, R. Paul, Crane, Jeffrey D., Shectman, Stephen A., Beletsky, Yuri, Shporer, Avi, Montet, Benjamin T., Burt, Jennifer A., Feinstein, Adina D., Flowers, Erin, Nandakumar, Sangeetha, Barbieri, Mauro, Corbett, Hank, Ratzloff, Jeffrey K., Galliher, Nathan, Chavez, Ramses Gonzalez, Vasquez, Alan, Glazier, Amy, Haislip, Joshua
HD 21749 is a bright ($V=8.1$ mag) K dwarf at 16 pc known to host an inner terrestrial planet HD 21749c as well as an outer sub-Neptune HD 21749b, both delivered by TESS. Follow-up spectroscopic observations measured the mass of HD 21749b to be $22.7
Externí odkaz:
http://arxiv.org/abs/2012.04873
Autor:
Teske, Johanna, Wang, Sharon Xuesong, Wolfgang, Angie, Gan, Tianjun, Plotnykov, Mykhaylo, Armstrong, David J., Butler, R. Paul, Cale, Bryson, Crane, Jeffrey D., Howard, Ward, Jensen, Eric L. N., Law, Nicholas, Shectman, Stephen A., Plavchan, Peter, Valencia, Diana, Vanderburg, Andrew, Ricker, George, Vanderspek, Roland, Latham, Dave W., Seager, Sara, Winn, Joshua W., Jenkins, Jon M., Adibekyan, Vardan, Barrado, David, Barros, Susana C. C., Benkhaldoun, Zouhair, Brown, David J. A., Bryant, Edward M., Burt, Jennifer, Caldwell, Douglas A., Charbonneau, David, Cloutier, Ryan, Collins, Karen A., Collins, Kevin I., Colon, Nicole D., Conti, Dennis M., Demangeon, Olivier D. S., Eastman, Jason D., Elmufti, Mohammed, Feng, Fabo, Flowers, Erin, Guerrero, Natalia M., Hojjatpanah, Saeed, Irwin, Jonathan M., Isopi, Giovanni, Lillo-Box, Jorge, Mallia, Franco, Massey, Bob, Mori, Mayuko, Mullally, Susan E., Narita, Norio, Nishiumi, Taku, Osborn, Ares, Paegert, Martin, de Leon, Jerome Pitogo, Quinn, Samuel N., Reefe, Michael, Schwarz, Richard P., Shporer, Avi, Soubkiou, Abderahmane, Sousa, Sérgio G., Stockdale, Chris, Strøm, Paul A., Tan, Thiam-Guan, Tenenbaum, Peter, Wheatley, Peter J., Wittrock, Justin, Yahalomi, Daniel A., Zohrabi, Farzaneh
$Kepler$ revealed that roughly one-third of Sun-like stars host planets orbiting within 100 days and between the size of Earth and Neptune. How do these planets form, what are they made of, and do they represent a continuous population or multiple po
Externí odkaz:
http://arxiv.org/abs/2011.11560
Autor:
Burt, Jennifer A., Nielsen, Louise D., Quinn, Samuel N., Mamajek, Eric E., Matthews, Elisabeth C., Zhou, George, Seidel, Julia V., Huang, Chelsea X., Lopez, Eric, Soto, Maritza, Otegi, Jon, Stassun, Keivan G., Kreidberg, Laura, Collins, Karen A., Eastman, Jason D., Rodriguez, Joseph E., Vanderburg, Andrew, Halverson, Samuel P., Teske, Johanna K., Wang, Sharon X., Butler, R. Paul, Bouchy, François, Dumusque, Xavier, Segransen, Damien, Shectman, Stephen A., Crane, Jeffrey D., Feng, Fabo, Montet, Benjamin T., Feinstein, Adina D., Beletski, Yuri, Flowers, Erin, Günther, Maximilian N., Daylan, Tansu, Collins, Kevin I., Conti, Dennis M., Gan, Tianjun, Jensen, Eric L. N., Kielkopf, John F., Tan, Thiam Guan, Helled, Ravit, Dorn, Caroline, Haldemann, Jonas, Lissauer, Jack J., Ricker, George R., Vanderspek, Roland, Latham, David W., Seager, S., Winn, Joshua N., Jenkins, Jon M., Twicken, Joseph D., Smith, Jeffrey C., Tenenbaum, Peter, Cartwright, Scott, Barclay, Thomas, Pepper, Joshua, Esquerdo, Gilbert, Fong, William
We report the detection of a transiting hot Neptune exoplanet orbiting TOI-824 (SCR J1448-5735), a nearby (d = 64 pc) K4V star, using data from the \textit{Transiting Exoplanet Survey Satellite} (TESS). The newly discovered planet has a radius, $R_{\
Externí odkaz:
http://arxiv.org/abs/2008.11732
Autor:
Teske, Johanna, Díaz, Matías R., Luque, Rafael, Močnik, Teo, Seidel, Julia V., Otegi, Jon Fernández, Feng, Fabo, Jenkins, James S., Pallè, Enric, Ségransan, Damien, Udry, Stèphane, Collins, Karen A., Eastman, Jason D., Ricker, George R., Vanderspek, Roland, Latham, David W., Seager, Sara, Winn, Joshua N., Jenkins, Jon M., Anderson, David. R., Barclay, Thomas, Bouchy, François, Burt, Jennifer A., Butler, R. Paul, Caldwell, Douglas A., Collins, Kevin I., Crane, Jeffrey D., Dorn, Caroline, Flowers, Erin, Haldemann, Jonas, Helled, Ravit, Hellier, Coel, Jensen, Eric L. N., Kane, Stephen R., Law, Nicholas, Lissauer, Jack J., Mann, Andrew W., Marmier, Maxime, Nielsen, Louise Dyregaard, Rose, Mark E., Shectman, Stephen A., Shporer, Avi, Torres, Guillermo, Wang, Sharon X., Wolfgang, Angie, Wong, Ian, Ziegler, Carl
The Transiting Exoplanet Survey Satellite mission was designed to find transiting planets around bright, nearby stars. Here we present the detection and mass measurement of a small, short-period ($\approx\,4$\,days) transiting planet around the brigh
Externí odkaz:
http://arxiv.org/abs/2007.13927
Autor:
Mireles, Ismael, Shporer, Avi, Grieves, Nolan, Zhou, George, Günther, Maximilian N., Brahm, Rafael, Ziegler, Carl, Stassun, Keivan G., Huang, Chelsea X., Nielsen, Louise, Santos, Leonardo A. dos, Udry, Stéphane, Bouchy, François, Ireland, Michael, Wallace, Alexander, Sarkis, Paula, Henning, Thomas, Jordan, Andres, Law, Nicholas, Mann, Andrew W., Paredes, Leonardo A., James, Hodari-Sadiki, Jao, Wei-Chun, Henry, Todd J., Butler, R. Paul, Rodriguez, Joseph E., Yu, Liang, Flowers, Erin, Ricker, George R., Latham, David W., Vanderspek, Roland, Seager, Sara, Winn, Joshua N., Jenkins, Jon M., Furesz, Gabor, Hesse, Katharine, Quintana, Elisa V., Rose, Mark E., Smith, Jeffrey C., Tenenbaum, Peter, Vezie, Michael, Yahalomi, Daniel A., Zhan, Zhuchang
We report the discovery of TOI 694 b and TIC 220568520 b, two low-mass stellar companions in eccentric orbits around metal-rich Sun-like stars, first detected by the Transiting Exoplanet Survey Satellite (TESS). TOI 694 b has an orbital period of 48.
Externí odkaz:
http://arxiv.org/abs/2006.14019
Autor:
Carleo, Ilaria, Gandolfi, Davide, Barragán, Oscar, Livingston, John H., Persson, Carina M., Lam, Kristine W. F., Vidotto, Aline, Lund, Michael B., D'Angelo, Carolina Villarreal, Collins, Karen A., Fossati, Luca, Howard, Andrew W., Kubyshkina, Daria, Brahm, Rafael, Oklopčić, Antonija, Mollière, Paul, Redfield, Seth, Serrano, Luisa Maria, Dai, Fei, Fridlund, Malcolm, Borsa, Francesco, Korth, Judith, Esposito, Massimiliano, Díaz, Matías R., Nielsen, Louise Dyregaard, Hellier, Coel, Mathur, Savita, Deeg, Hans J., Hatzes, Artie P., Benatti, Serena, Rodler, Florian, Alarcon, Javier, Spina, Lorenzo, Santos, Ângela R. G., Georgieva, Iskra, García, Rafael A., González-Cuesta, Lucía, Ricker, George R., Vanderspek, Roland, Latham, David W., Seager, Sara, Winn, Joshua N., Jenkins, Jon M., Albrecht, Simon, Batalha, Natalie M., Beard, Corey, Boyd, Patricia T., Bouchy, François, Burt, Jennifer A., Butler, R. Paul, Cabrera, Juan, Chontos, Ashley, Ciardi, David, Cochran, William D., Collins, Kevin I., Crane, Jeffrey D., Crossfield, Ian, Csizmadia, Szilard, Dragomir, Diana, Dressing, Courtney, Eigmüller, Philipp, Endl, Michael, Erikson, Anders, Espinoza, Nestor, Fausnaugh, Michael, Feng, Fabo, Flowers, Erin, Fulton, Benjamin, Gonzales, Erica J., Grieves, Nolan, Grziwa, Sascha, Guenther, Eike W., Guerrero, Natalia M., Henning, Thomas, Hidalgo, Diego, Hirano, Teruyuki, Hjorth, Maria, Huber, Daniel, Isaacson, Howard, Jones, Matias, Jordán, Andrés, Kabáth, Petr, Kane, Stephen R., Knudstrup, Emil, Lubin, Jack, Luque, Rafael, Mireles, Ismael, Narita, Norio, Nespral, David, Niraula, Prajwal, Nowak, Grzegorz, Palle, Enric, Pätzold, Martin, Petigura, Erik A, Prieto-Arranz, Jorge, Rauer, Heike, Robertson, Paul, Rose, Mark E., Roy, Arpita, Sarkis, Paula, Schlieder, Joshua E., Ségransan, Damien, Shectman, Stephen, Skarka, Marek, Smith, Alexis M. S., Smith, Jeffrey C., Stassun, Keivan, Teske, Johanna, Twicken, Joseph D., Van Eylen, Vincent, Wang, Sharon, Weiss, Lauren M., Wyttenbach, Aurélien
Publikováno v:
2020AJ....160..114C
We report the discovery of a warm Neptune and a hot sub-Neptune transiting TOI-421 (BD-14 1137, TIC 94986319), a bright (V=9.9) G9 dwarf star in a visual binary system observed by the TESS space mission in Sectors 5 and 6. We performed ground-based f
Externí odkaz:
http://arxiv.org/abs/2004.10095
Autor:
Montet, Benjamin T., Feinstein, Adina D., Luger, Rodrigo, Bedell, Megan E., Gully-Santiago, Michael A., Teske, Johanna K., Wang, Sharon Xuesong, Butler, R. Paul, Flowers, Erin, Shectman, Stephen A., Crane, Jeffrey D., Thompson, Ian B.
The abundance of short-period planetary systems with high orbital obliquities relative to the spin of their host stars is often taken as evidence that scattering processes play important roles in the formation and evolution of these systems. More rec
Externí odkaz:
http://arxiv.org/abs/1912.03794
The signature of wind patterns caused by the interplay of rotation and energy redistribution in hot Jupiters is detectable at high spectral resolution, yet no direct comparison has been attempted between predictions from general circulation models (G
Externí odkaz:
http://arxiv.org/abs/1810.06099