Zobrazeno 1 - 10
of 108
pro vyhledávání: '"Arne Henden"'
Autor:
Golovin, Alex, Kazuya, Ayani, P., Pavlenko Elena, Tom, Krajci, Yuliana, Kuznyetsova, Arne, Henden, Victoria, Krushevska, Shawn, Dvorak, Kirill, Sokolovsky, P., Sergeeva Tatyana, Robert, James, Tim, Crawford, Laurent, Corp
Publikováno v:
2007IBVS.5763....1G
We report CCD photometry and spectroscopy during 2006 outburst of the dwarf nova SDSS J102146.44+234926.3 (SDSS J1021). The photographic plates from the MAO, SAI and CrAO plate archives, which cover the position of the SDSS J1021, were inspected for
Externí odkaz:
http://arxiv.org/abs/0704.1276
Autor:
Rachel B. Fernandes, William C. Danchi, Evan A. Rich, Carol A. Grady, Zachary C. Long, Arne Henden, Korash Assani, Michael L. Sitko, John P. Wisniewski, Ammar Bayyari, Monika Pikhartova
HD 163296 is a Herbig Ae star that underwent a dramatic $\sim$0.8 magnitude drop in brightness in the V photometric band in 2001 and a brightening in the near-IR in 2002. Because the star possesses Herbig-Haro objects travelling in outflowing bipolar
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5eef328b725764d51cf45bcfb8a3f6fa
Autor:
Nicolas F. Martin, Luca Sbordone, R. G. Carlberg, K. A. Venn, Pascale Jablonka, Julio F. Navarro, Anke Arentsen, Else Starkenburg, Stefania Salvadori, Arne Henden, Carmela Lardo, David Aguado, Rubén Sánchez-Janssen, P. Bonifacio, J. I. González Hernández, P. Francois, Elisabetta Caffau, Federico Sestito, V. Hill
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, In press, 487 (3), pp.3797-3814. ⟨10.1093/mnras/stz1378⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, In press, 487 (3), pp.3797-3814. ⟨10.1093/mnras/stz1378⟩
With the aim of probing the properties of the bright end of the Pristine survey and its effectiveness in selecting metal-poor stars, we selected a sample of bright candidate metal-poor stars combining Pristine CaHK photometry with APASS gi photometry
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::49cdccafde3e021cca748b4bc50d12a5
https://hal.archives-ouvertes.fr/hal-02138411/file/sophie.pdf
https://hal.archives-ouvertes.fr/hal-02138411/file/sophie.pdf
Autor:
Thomas W.-S. Holoien, Joshua D. Simon, Christopher S. Kochanek, Jennifer L. van Saders, Arne Henden, Benjamin J. Shappee, G. Pojmanski, Benjamin T. Montet
We present ~800 days of photometric monitoring of Boyajian's Star (KIC 8462852) from the All-Sky Automated Survey for Supernovae (ASAS-SN) and ~4000 days of monitoring from the All Sky Automated Survey (ASAS). We show that from 2015 to the present th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::009ce8400f8f95d265f2ef246623dec6
Publikováno v:
New Astronomy. 27:1-12
The Aquarius stream has been recently discovered in the course of the RAVE Survey. It is a chemically coherent structure, originating from the tidal disruption of a 12 Gyr, [Fe/H] = −1.0 globular cluster. We have surveyed a ∼ 284 deg2 area of the
Publikováno v:
New Astronomy. 20:30-37
Accurate and densely populated BVRcIc lightcurves of supernovae SN 2011fe in M101, SN 2012aw in M95 and SN 2012cg in NGC 4424 are presented and discussed. The SN 2011fe lightcurve spans a total range of 342 days, from 17 days pre- to 325 days post-ma
Autor:
David D. Balam, Joanne M. Rosvick, Daniel J. Majaess, Arne Henden, David G. Turner, David J. Lane
Publikováno v:
Publications of the Astronomical Society of the Pacific. 123:1249-1261
The likely membership of the planetary nebula Abell 8 (PN G167.0--00.9) in the open cluster Bica 6 is confirmed by CCD spectra, UBV(RI)c photometry, and radial velocities for luminous cluster stars. The reddening, estimated distance, and radial veloc
Survey of Period Variations of Superhumps in SU UMa-Type Dwarf Novae. II The Second Year (2009–2010)
Autor:
Enrique de Miguel, Katsura Matsumoto, Pavol A. Dubovsky, Kousei Yamashita, Shinichi Nakagawa, Arne Henden, Rod Stubbings, Daichi Fujii, Christopher Stockdale, Igor Kudzej, Kazuyoshi Imamura, Ryoko Ishioka, Daisaku Nogami, David Boyd, Etienne Morelle, Tim Crawford, F. A. Ringwald, Nanae Kunitomi, Peter Nelson, Akira Imada, Makoto Uemura, Roger D. Pickard, Bart Staels, Kenji Tanabe, Seiichiro Kiyota, Arto Oksanen, Eriko Iino, Elena P. Pavlenko, Ryo Noguchi, Eddy Muyllaert, Hiroshi Itoh, Rudolf Novak, Gianluca Masi, Taichi Kato, Mike Simonsen, Sachi Ohtomo, Michael Richmond, Tetsuya Kuramoto, Hiroyuki Maehara, Steve Brady, Atsushi Miyashita, Tomas Hynek, Tomohito Ohshima, Hirofumi Yanagisawa, Tomás L. Gómez, Shawn Dvorak, Javier Ruiz, Kazuyuki Ogura, Hiroshi Kobayashi, Irina Voloshina, Ian Miller, Ryosuke Takagi, Franz-Josef Hambsch, Greg Bolt, Mikiha Nose, Jeremy Shears, Berto Monard, Thomas Krajci, Hidehiko Akazawa
Publikováno v:
Publications of the Astronomical Society of Japan. 62:1525-1584
As an extension of the project in Kato et al. (2009, arXiv:0905.1757), we collected times of superhump maxima for 61 SU UMa-type dwarf novae mainly observed during the 2009-2010 season. The newly obtained data confirmed the basic findings reported in
Publikováno v:
The Astronomical Journal. 139:1527-1533
We present data from the archival plates at Harvard College Observatory and Sonneberg Observatory showing the field of the solar type pre-main sequence star GM Cep. A total of 186 magnitudes of GM Cep have been measured on these archival plates, with