Zobrazeno 1 - 10
of 165
pro vyhledávání: '"Kenneth H. Hinkle"'
Autor:
Kenneth H. Hinkle, Francis C. Fekel, Oscar Straniero, Zachary G. Maas, Richard R. Joyce, Thomas Lebzelter, Matthew W. Muterspaugh, James R. Sowell
Publikováno v:
The Astrophysical Journal, Vol 969, Iss 1, p 35 (2024)
A single-lined spectroscopic orbit for the M giant in the X-ray binary IGR J16194−2810 is determined from a time series of optical spectra. The spectroscopic orbital period of 192.5 days is twice that of the photometric period, confirming that the
Externí odkaz:
https://doaj.org/article/2735d8ed7f6b423f9b845b9cfc468ef2
Publikováno v:
The Astrophysical Journal. 937:98
The Mira in the bright, dusty, symbiotic binary R Aquarii undergoes eclipses of multiyear duration every ∼44 yr by a large, opaque accretion disk. The 2020 eclipse was confirmed by I-band photometry. High-resolution M- and K-band spectra were obser
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ad96321850873976a3235dd508f42313
https://doi.org/10.3847/1538-4357/ac8a47
https://doi.org/10.3847/1538-4357/ac8a47
Publikováno v:
Proceedings of the International Astronomical Union. 15:211-214
Masses have been computed for the white dwarfs (WDs) in eclipsing, mass exchange (symbiotic), WD–red giant (RG) binaries by using single-lined spectroscopic orbits, orbital inclinations, and the RG masses. Inclinations have been measured for 13 ecl
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::be90e1f7300b9f47ece57f4ccc04c035
https://doi.org/10.1017/s174392132000068x
https://doi.org/10.1017/s174392132000068x
The infrared view of dust and molecules around V4334 Sgr (Sakurai’s Object): a 20-year retrospective
Autor:
Joachim Krautter, S. P. S. Eyres, L. A. Helton, E. Montiel, Matthew J. Richter, Peter J. Sarre, T. Liimets, Kenneth H. Hinkle, Foteini Lykou, Chick E Woodward, Hannah L. Worters, S. G. Starrfield, Robert D. Gehrz, Debabrata Banerjee, Geoffrey C. Clayton, A. A. Zijlstra, Richard R. Joyce, Thomas R. Geballe, A. Evans
Publikováno v:
Evans, A, Gehrz, R D, Woodward, C E, Banerjee, D P K, Geballe, T R, Clayton, G C, Sarre, P J, Starrfield, S, Hinkle, K, Joyce, R R, Lykou, F, Helton, L A, Eyres, S P S, Worters, H, Montiel, E J, Liimets, T, Zijlstra, A, Richter, M & Krautter, J 2020, ' The infrared view of dust and molecules around V4334 Sgr (Sakurai’s Object): a 20-year retrospective ', Monthly Notices of the Royal Astronomical Society . https://doi.org/10.1093/mnras/staa343
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society
We present an analysis of the evolution of circumstellar dust and molecules in the environment of the very late thermal pulse object V4334 Sgr (Sakurai's Object) over a $\sim20$-year period, drawing on ground-, airborne- and space-based infrared phot
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7a6eb8bd2a6ce645ca2e4dc0cef3cba8
https://pure.manchester.ac.uk/ws/files/159126346/Sak_dust_mol_in_press.pdf
https://pure.manchester.ac.uk/ws/files/159126346/Sak_dust_mol_in_press.pdf
Autor:
Oscar Straniero, Kenneth H. Hinkle, Lisa Prato, Thomas Lebzelter, Nolan M. Habel, Nicole Karnath, Francis C. Fekel, Richard R. Joyce
The X-ray binary 4U 1954+31 has been classified as a Low Mass X-ray Binary (LMXB) containing a M giant and a neutron star (NS). It has also been included in the rare class of X-ray symbiotic binaries (SyXB). The Gaia parallax, infrared colors, spectr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::403c49269896d107dc9086357d2d361f
Chemical abundance analysis of 13 southern symbiotic giants from high-resolution spectra at ∼1.56 μm
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 466:2194-2201
Symbiotic stars (SySt) are binaries composed of a star in the later stages of evolution and a stellar remnant. The enhanced mass-loss from the giant drives interacting mass exchange and makes these systems laboratories for understanding binary evolut
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bfc6355da082d055ff2165d4da294dc8
https://doi.org/10.1093/mnras/stw3266
https://doi.org/10.1093/mnras/stw3266
Publikováno v:
Proceedings of the International Astronomical Union. 14:495-497
The carbon-rich AGB star V Hya is believed to be in the very brief transition phase between the AGB and a planetary nebula (PN). Using HST/STIS, we previously found a high-velocity (> 200 kms−1) jet or blob of gas ejected only a few years ago from
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::586778a801f7472acc30c67f4ceb97b0
https://doi.org/10.1017/s1743921318007172
https://doi.org/10.1017/s1743921318007172
Autor:
Oscar Straniero, Thomas Lebzelter, Kenneth H. Hinkle, Kristie A. Nault, Catherine A. Pilachowski, David L. Lambert
Carbon and oxygen isotopic ratios are reported for a sample of 51 SRb- and Lb-type variable asymptotic giant branch stars. Vibration-rotation first- and second-overtone CO lines in 1.5-2.5 mum spectra were measured to derive isotopic ratios for 12C/1
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1bd3271b27660b7292b47243505d6694
Publikováno v:
The Astrophysical Journal. 904:34
Observations of the ejecta from the final flash (FF) of helium shell burning in Sakurai’s Object (V4334 Sgr) are presented for 2015–2019, a period ∼20–24 yr after discovery. Adaptive optics images at K s trace the expanding debris. While most
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9441a8f6bdfb7fbdedae544a6f5792d9
https://doi.org/10.3847/1538-4357/abbd9a
https://doi.org/10.3847/1538-4357/abbd9a
Autor:
S. G. Starrfield, Matthew J. Richter, Debabrata Banerjee, Richard R. Joyce, S. P. S. Eyres, A. Evans, Charles E. Woodward, T. Liimets, E. Montiel, Curtis DeWitt, Kenneth H. Hinkle, R. M. Wagner, Robert D. Gehrz, Hannah L. Worters, Geoffrey C. Clayton
Publikováno v:
The Astronomical Journal. 159:87
Large aromatic molecules are ubiquitous in both circumstellar and interstellar environments. Detection of small aromatic molecules, such as benzene (C6H6) and benzyne (C6H4), are rare in astrophysical environments. Detection of such species will have
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::99f90e4b689619522c00d1e337823ef0
https://doi.org/10.3847/1538-3881/ab67c2
https://doi.org/10.3847/1538-3881/ab67c2