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Artículos de revistas sobre el tema "HD"

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Publicado: 4 de junio de 2021
Última modificación: 25 de julio de 2025

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1

Koga, Hisao, Akira Atsuta, and Michimasa Aramaki. "HD-PLC." Journal of The Institute of Image Information and Television Engineers 64, no. 11 (2010): 1580–83. http://dx.doi.org/10.3169/itej.64.1580.

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2

Dukes, Robert J., and Saul J. Adelman. "Studies of FCAPT uvby Photometry with Period04: The mCP Stars HD 5797, HD 36792, HD 27309, HD 47913, HD 74521, HD 120198, HD 171263, and HD 215441." Publications of the Astronomical Society of the Pacific 130, no. 986 (2018): 044202. http://dx.doi.org/10.1088/1538-3873/aaa952.

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3

Monier, R., M. Gebran, and F. Royer. "Four new HgMn stars: HD 18104, HD 30085, HD 32867, and HD 53588." Astronomy & Astrophysics 577 (May 2015): A96. http://dx.doi.org/10.1051/0004-6361/201526106.

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4

Jones, H. R. A., R. Paul Butler, G. W. Marcy, et al. "Extrasolar planets around HD 196050, HD 216437 and HD 160691." Monthly Notices of the Royal Astronomical Society 337, no. 4 (2002): 1170–78. http://dx.doi.org/10.1046/j.1365-8711.2002.05787.x.

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5

Глаголевский, Ю. В. "Структуры магнитного поля звезд HD 94660, HD 75049, HD 154708". Pisʹma v Astronomičeskij žurnal 50, № 2 (2024): 172–79. http://dx.doi.org/10.31857/s0320010824020041.

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6

Fischer, Debra A., Geoffrey W. Marcy, R. Paul Butler, Steven S. Vogt, Bernie Walp, and Kevin Apps. "Planetary Companions to HD 136118, HD 50554, and HD 106252." Publications of the Astronomical Society of the Pacific 114, no. 795 (2002): 529–35. http://dx.doi.org/10.1086/341677.

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7

McKellar, A. R. W. "Interference effects in the spectrum of HD: VI: HD–HD, and HD–Kr at room temperature." Canadian Journal of Physics 72, no. 5-6 (1994): 215–24. http://dx.doi.org/10.1139/p94-033.

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The absorption spectrum of the fundamental band of hydrogen deuteride (λ ≈ 2.7 μm) has been studied in pure HD and in mixtures with krypton at moderate densities (1–45 amagat) and room temperature, using a high-resolution Fourier transform infrared spectrometer. The effects that arise from interference between the allowed dipole transition moments of free HD and the dipoles induced during collisions were studied. For HD–HD collisions, the eight transitions from P1(3) to R1(4) were analyzed to determine line positions, intensities, shift and broadening coefficients, and the phase shift paramete
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8

LeBlanc, F., V. Khalack, B. Yameogo, C. Thibeault, and I. Gallant. "Project VeSElkA: results of abundance analysis I – HD 71030, HD 95608, HD 116235 and HD 186568." Monthly Notices of the Royal Astronomical Society 453, no. 4 (2015): 3767–72. http://dx.doi.org/10.1093/mnras/stv1466.

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9

Stateva, I., I. Kh Iliev, and J. Budaj. "Abundance analysis of Am binaries and search for tidally driven abundance anomalies - III. HD 116657, HD 138213, HD 155375, HD 159560, HD 196544 and HD 204188." Monthly Notices of the Royal Astronomical Society 420, no. 2 (2011): 1207–16. http://dx.doi.org/10.1111/j.1365-2966.2011.20108.x.

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10

Iliev, I. K., J. Budaj, M. Fenovcik, I. Stateva, and M. T. Richards. "Abundance analysis of Am binaries and search for tidally driven abundance anomalies - II. HD 861, HD 18778, HD 20320, HD 29479, HD 96528 and HD 108651." Monthly Notices of the Royal Astronomical Society 370, no. 2 (2006): 819–27. http://dx.doi.org/10.1111/j.1365-2966.2006.10513.x.

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11

Sadakane, Kozo, Takashi Ohnishi, Michiko Ohkubo, and Yoichi Takeda. "Metallicities in Four Planet-Harbouring K-Type Giants: HD 47536, HD 59686, HD 137759, and HD 219449." Publications of the Astronomical Society of Japan 57, no. 1 (2005): 127–33. http://dx.doi.org/10.1093/pasj/57.1.127.

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12

Giguere, Matthew J., Debra A. Fischer, Matthew J. Payne, et al. "NEWLY DISCOVERED PLANETS ORBITING HD 5319, HD 11506, HD 75784 AND HD 10442 FROM THE N2K CONSORTIUM." Astrophysical Journal 799, no. 1 (2015): 89. http://dx.doi.org/10.1088/0004-637x/799/1/89.

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13

Перминов, А. С., та Э. Д. Кузнецов. "Орбитальная эволюция внесолнечных планетных систем HD 39194, HD 141399 и HD 160691". Астрономический журнал 96, № 10 (2019): 795–814. http://dx.doi.org/10.1134/s000462991909007x.

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14

Kiseleva-Eggleton, Ludmila, Eric Bois, Nicolas Rambaux, and Rudolf Dvorak. "Global Dynamics and Stability Limits for Planetary Systems around HD 12661, HD 38529, HD 37124, and HD 160691." Astrophysical Journal 578, no. 2 (2002): L145—L148. http://dx.doi.org/10.1086/344706.

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15

Jeong, Gwanghui, Inwoo Han, Myeong-Gu Park, et al. "A Search for Exoplanets around Northern Circumpolar Stars. IV. Six Planet Candidates to the K Giants, HD 44385, HD 97619, HD 106574, HD 118904, HD 164428, and HD 202432." Astronomical Journal 156, no. 2 (2018): 64. http://dx.doi.org/10.3847/1538-3881/aacbc1.

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16

Ment, Kristo, Debra A. Fischer, Gaspar Bakos, Andrew W. Howard, and Howard Isaacson. "Radial Velocities from the N2K Project: Six New Cold Gas Giant Planets Orbiting HD 55696, HD 98736, HD 148164, HD 203473, and HD 211810." Astronomical Journal 156, no. 5 (2018): 213. http://dx.doi.org/10.3847/1538-3881/aae1f5.

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17

Procházka, Robert. "Anal intraepithelial neoplasia and HD anoscopy." Gastroenterologie a hepatologie 75, no. 3 (2021): 229–33. http://dx.doi.org/10.48095/ccgh2021229.

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Anal intraepithelial neoplasia (AIN) is a precursor lesion of anal squamous cell cancer (aSCC). aSCC is considered a rare cancer, but its incidence is on the rise and in certain high-risk populations it approaches the incidence of colorectal cancer. Although controlled randomized trials are lacking, expert opinions support screening and therapy of this anal neoplasia in the high-risk groups. AIN/aSCC belongs among neoplasia associated with HPV infection. Individuals with a higher AIN/aSCC risk can be examined by rectal smear for cytology or more sensitive HPV DNA, not unlike the cervical cance
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18

Karinkuzhi, Drisya, Aruna Goswami, Navin Sridhar, Thomas Masseron, and Meenakshi Purandardas. "Chemical analysis of three barium stars: HD 51959, HD 88035, and HD 121447." Monthly Notices of the Royal Astronomical Society 476, no. 3 (2018): 3086–96. http://dx.doi.org/10.1093/mnras/sty320.

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19

Gruberbauer, M., D. Huber, R. Kuschnig, et al. "MOST observations of the roAp stars HD 9289, HD 99563, and HD 134214." Astronomy & Astrophysics 530 (May 25, 2011): A135. http://dx.doi.org/10.1051/0004-6361/201116736.

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20

Glagolevskij, Yu V. "Magnetic Field Structures of the Stars HD 94660, HD 75049, and HD 154708." Astronomy Letters 50, no. 2 (2024): 148–58. http://dx.doi.org/10.1134/s106377372470004x.

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21

Halbedel, Elaine M. "Photometry of three Herbig Be stars - HD 53367, HD 200775, and HD 259431." Publications of the Astronomical Society of the Pacific 101 (November 1989): 1004. http://dx.doi.org/10.1086/132567.

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22

Sun, Sining, and Maria-Eirini Pandelia. "HD-[HD-GYP] Phosphodiesterases: Activities and Evolutionary Diversification within the HD-GYP Family." Biochemistry 59, no. 25 (2020): 2340–50. http://dx.doi.org/10.1021/acs.biochem.0c00257.

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23

Lester, Kathryn V., Gail H. Schaefer, Francis C. Fekel, et al. "Visual Orbits of Spectroscopic Binaries with the CHARA Array. IV. HD 61859, HD 89822, HD 109510, and HD 191692." Astronomical Journal 164, no. 6 (2022): 228. http://dx.doi.org/10.3847/1538-3881/ac9385.

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Abstract We present the visual orbits of four spectroscopic binary stars, HD 61859, HD 89822, HD 109510, and HD 191692, using long baseline interferometry with the CHARA Array. We also obtained new radial velocities from echelle spectra using the APO 3.5 m, CTIO 1.5 m, and Fairborn Observatory 2.0 m telescopes. By combining the astrometric and spectroscopic observations, we solve for the full, three-dimensional orbits and determine the stellar masses to 1%–12% uncertainty and distances to 0.4%–6% uncertainty. We then estimate the effective temperature and radius of each component star through
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24

Peterson, R. C., B. Barbuy, and M. Spite. "Trans-iron Ge, As, Se, and heavier elements in the dwarf metal-poor stars HD 19445, HD 84937, HD 94028, HD 140283, and HD 160617." Astronomy & Astrophysics 638 (June 2020): A64. http://dx.doi.org/10.1051/0004-6361/202037689.

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Context. The spectra of unevolved metal-poor halo stars uniquely reflect the elemental abundances incorporated during the earliest Galactic epoch. Their heavy-element content is well understood as the products of neutron capture on iron-peak elements. However, for the lightest trans-iron elements with atomic number 30 < Z < 52, they show striking abundance patterns that defy model predictions. Understanding their sources may illuminate the diverse halo, thick disk, or extragalactic origins of metal-poor stars. Aims. The primary goal is the derivation of halo dwarf abundances and their un
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25

Sinitskii, L. A., and I. M. Romanishin. "HD-Systems." Journal of Automation and Information Sciences 30, no. 1 (1998): 82–95. http://dx.doi.org/10.1615/jautomatinfscien.v30.i1.70.

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26

Arora, Akhil, Sakshi Sinha, Piyush Kumar, and Arnab Bhattacharya. "HD-index." Proceedings of the VLDB Endowment 11, no. 8 (2018): 906–19. http://dx.doi.org/10.14778/3204028.3204034.

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27

Fuhry, David, Yang Zhang, Venu Satuluri, Arnab Nandi, and Srinivasan Parthasarathy. "PLASMA-HD." Proceedings of the VLDB Endowment 6, no. 12 (2013): 1318–21. http://dx.doi.org/10.14778/2536274.2536305.

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28

Flaxton, Terry. "HD Aesthetics." Convergence: The International Journal of Research into New Media Technologies 17, no. 2 (2011): 113–23. http://dx.doi.org/10.1177/1354856510394884.

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29

VEATCHGOODMAN, L., P. COMO, J. CHA, and J. PAULSEN. "Treatment of HD: A Survey of HD Clinicians." Neurotherapeutics 5, no. 2 (2008): 374. http://dx.doi.org/10.1016/j.nurt.2007.10.047.

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30

McCarthy, Chris, R. Paul Butler, C. G. Tinney, et al. "Multiple Companions to HD 154857 and HD 160691." Astrophysical Journal 617, no. 1 (2004): 575–79. http://dx.doi.org/10.1086/425214.

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31

Kremer, H. P. H. "Imaging Huntington's disease (HD) brains - imagine HD trials!" Journal of Neurology, Neurosurgery & Psychiatry 76, no. 5 (2005): 620. http://dx.doi.org/10.1136/jnnp.2004.056267.

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32

Perminov, A. S., and E. D. Kuznetsov. "Orbital Evolution of the Extrasolar Planetary Systems HD 39194, HD 141399, and HD 160691." Astronomy Reports 63, no. 10 (2019): 795–813. http://dx.doi.org/10.1134/s1063772919090075.

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33

Miller, Ricarda E., Toni Rantanen, Kevin A. Ogilvie, Ulrich Groth, and Victor Snieckus. "Combined DirectedorthoMetalation−Halogen Dance (HD) Synthetic Strategies. HD−AnionicorthoFries Rearrangement and Double HD Sequences." Organic Letters 12, no. 10 (2010): 2198–201. http://dx.doi.org/10.1021/ol100493v.

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34

Jeong, G., B. C. Lee, I. Han, et al. "Detection of planet candidates around K giants. HD 40956, HD 111591, and HD 113996." Astronomy & Astrophysics 610 (February 2018): A3. http://dx.doi.org/10.1051/0004-6361/201629185.

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Aims. The purpose of this paper is to detect and investigate the nature of long-term radial velocity (RV) variations of K-type giants and to confirm planetary companions around the stars. Methods. We have conducted two planet search programs by precise RV measurement using the 1.8 m telescope at Bohyunsan Optical Astronomy Observatory (BOAO) and the 1.88 m telescope at Okayama Astrophysical Observatory (OAO). The BOAO program searches for planets around 55 early K giants. The OAO program is looking for 190 G–K type giants. Results. In this paper, we report the detection of long-period RV varia
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35

Holanda, N., T. Flaulhabe, F. Quispe-Huaynasi, A. Sonally, and C. B. Pereira. "The Chemical Puzzle of Weak G-Band Stars: A Comprehensive Study of HD 54627, HD 105783, HD 198718, and HD 201557." Astrophysical Journal 971, no. 2 (2024): 152. http://dx.doi.org/10.3847/1538-4357/ad58bf.

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Abstract Weak G-band stars (WGBs) are a unique class of objects characterized by weak CH molecular lines in the Fraunhofer G band, indicative of a deficiency in 12C. This peculiar spectral feature is often accompanied by significant enrichments in N and, occasionally, Li and Na abundances. Despite their rarity and recent discoveries of new WGB candidates, the underlying formation mechanism of these stars remains unknown. In this study, we present a comprehensive chemical analysis of four neglected WGBs: HD 54627, HD 105783, HD 198718, and HD 201557. These stars, though identified as WGBs, have
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36

JEON, YOUNG-BEOM, KI-HYUNG NAM, SEUNG-LEE KIM та ін. "A NEW FIELD δ SCUTI STAR: HD 235428". Publications of The Korean Astronomical Society 19, № 1 (2004): 27–31. http://dx.doi.org/10.5303/pkas.2004.19.1.027.

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37

Glagolevskij, Yu V. "Structure of the Magnetic Field of Massive O Stars HD 37022, HD 191612, HD 149438." Astrophysical Bulletin 79, no. 2 (2024): 260–74. http://dx.doi.org/10.1134/s1990341324600595.

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38

Glagolevskij, Yurij V., and Ewald Gerth. "Modelling of three long-periodic magnetic CP-stars: HD 2453, HD 12288, and HD 200311." Proceedings of the International Astronomical Union 2004, IAUS224 (2004): 614–18. http://dx.doi.org/10.1017/s1743921305009440.

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39

King, J. R. "Lithium Abundances of the Cool Metal-Poor Dwarfs HD 103095, HD 134439, and HD 134440." Publications of the Astronomical Society of the Pacific 109 (July 1997): 776. http://dx.doi.org/10.1086/133943.

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40

Fischer, Debra A., Geoffrey W. Marcy, R. Paul Butler, et al. "A Planetary Companion to HD 40979 and Additional Planets Orbiting HD 12661 and HD 38529." Astrophysical Journal 586, no. 2 (2003): 1394–408. http://dx.doi.org/10.1086/367889.

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41

Романовская, А. М., Т. А. Рябчикова та Д. В. Шуляк. "Эволюционный статус Ар-звезд HD 110066 и HD 153882". Письма в астрономический журнал: Астрономия и космическая астрофизика 46, № 05 (2020): 353–65. http://dx.doi.org/10.31857/s032001082005006x.

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42

Downing, Nancy R., Spencer Lourens, Isabella De Soriano, Jeffrey D. Long, and Jane S. Paulsen. "Phenotype Characterization of HD Intermediate Alleles in PREDICT-HD." Journal of Huntington's Disease 5, no. 4 (2016): 357–68. http://dx.doi.org/10.3233/jhd-160185.

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43

Boyajian, T. S., T. D. Beaulieu, D. R. Gies, et al. "The Massive Runaway Stars HD 14633 and HD 15137." Astrophysical Journal 621, no. 2 (2005): 978–84. http://dx.doi.org/10.1086/427650.

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44

Helling, Ch, G. Lee, I. Dobbs-Dixon, et al. "The mineral clouds on HD 209458b and HD 189733b." Monthly Notices of the Royal Astronomical Society 460, no. 1 (2016): 855–83. http://dx.doi.org/10.1093/mnras/stw662.

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45

Hall, Douglas S., and Gregory W. Henry. "Two New Spotted Variables-HD 191262 and HD 191011." Astronomical Journal 104 (November 1992): 1936. http://dx.doi.org/10.1086/116369.

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46

Strasburger, Krzysztof. "Modified adiabatic approximation: Charge asymmetry in HD+ and HD." Journal of Chemical Physics 131, no. 13 (2009): 134103. http://dx.doi.org/10.1063/1.3241280.

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47

Lu, Wen-xian. "Revised spectroscopic orbits of HD 144515 and HD 178428." Chinese Astronomy and Astrophysics 14, no. 3 (1990): 282–88. http://dx.doi.org/10.1016/0275-1062(90)90053-g.

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48

Glagolevskii, Yu V. "Magnetic field models for HD 116458 and HD 126515." Astronomy Reports 49, no. 12 (2005): 1001–8. http://dx.doi.org/10.1134/1.2139816.

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49

Pompéia, L., and D. M. Allen. "HD 11397 and HD 14282: two new barium stars?" Astronomy & Astrophysics 488, no. 2 (2008): 723–29. http://dx.doi.org/10.1051/0004-6361:200809707.

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50

Griffin, R. F., and Francis C. Fekel. "HD 115781 and HD 116204—two RS CVn binaries." Journal of Astrophysics and Astronomy 9, no. 4 (1988): 213–24. http://dx.doi.org/10.1007/bf02715066.

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