Results 31 to 40 of about 126,126 (337)
Variable stars in the northern Galactic plane from KISOGP
EPJ Web of Conferences, 2017 We have conducted a large-scale survey of the northern plane using KisoWide Field Camera attached to Schmidt telescope at Kiso Observatory. The KISOGP (KWFC Intensive Survey of the Galactic Plane) project has made 40–70 epoch observations in I band of ...Matsunaga Noriyukidoaj +1 more sourceAbsolute Proper Motions of H2O Masers Away from the Galactic Plane
Measured with VERA in the "Superbubble" Region NGC 281
, 2007 We report on absolute proper-motion measurements of an H2O maser source in
the NGC 281 West molecular cloud, which is located ~320 pc above the Galactic
plane and is associated with an HI loop extending from the Galactic plane.Bushimata, Takeshi, Choi, Yoon Kyung, Hirota, Tomoya, Honma, Mareki, Imai, Hiroshi, Iwadate, Kenzaburo, Jike, Takaaki, Kameno, Seiji, Kameya, Osamu, Kamohara, Ryuichi, Kan-ya, Yukitoshi, Kawaguchi, Noriyuki, Kijima, Masachika, Kim, Mi Kyoung, Kobayashi, Hideyuki, Kuji, Seisuke, Kurayama, Tomoharu, Manabe, Seiji, Maruyama, Kenta, Matsui, Makoto, Matsumoto, Naoko, Miyaji, Takeshi, Nagayama, Takumi, Nakagawa, Akiharu, Nakamura, Kayoko, Oh, Chung Sik, Omodaka, Toshihiro, Oyama, Tomoaki, Sakai, Satoshi, Sasao, Tetsuo, Sato, Katsuhisa, Sato, Mayumi, Shibata, Katsunori M., Shintani, Motonobu, Tamura, Yoshiaki, Tsushima, Miyuki, Yamashita, Kazuyoshi +36 morecore +2 more sourcesNew Galactic plane supernova remnants
The Astronomical Journal, 1992 A survey of the region 44° < l < 90°, |b| < 1.5° has been nearly completed using the Westerbork Synthesis Radio Telescope (WSRT) at 327 MHz. The low frequency, high resolution, and high sensitivity of this survey make it ideal for detecting supernova remnants (SNR's) which previous, primarily single dish, surveys have missed.A. R. Taylor, B. J. Wallace, W. M. Gossopenaire +1 more sourceThe Distribution of Open Clusters in the Galaxy
Frontiers in Astronomy and Space Sciences, 2021 In this work we explore the new catalog of galactic open clusters that became available recently, containing 1,750 clusters that have been re-analyzed using the Gaia DR2 catalog to determine the stellar memberships.Hektor Monteiro, Douglas A. Barros, Wilton S. Dias, Jacques R. D. Lépine +3 moredoaj +1 more sourceInterstellar extinction towards open clusters and galactic structure
, 2005 We study the distribution of interstellar matter near the galactic plane on
the basis of open star clusters and reviewed the correlation of extinction with
different physical parameters of the clusters to understand the galactic
structure.Arce, Arenou, Bica, Binney, Cambrésy, Cambrésy, Chen, Chen, Cohen, Conti, Dias, Dutra, Dutra, Dutra, Fernie, FitzGerald, Gum, Humphreys, Janes, Janes, Lockman, Lynga, Lynga, Lynga, Magnani, Martin, Maíz-Apellániz, Mermilliod, Méndez, Neckel, Neckel, Pandey, Pandey, Reed, Schlegel, Stenholm, Tarantola, Y. C. Joshi +37 morecore +1 more sourceIron Emission Lines on the Galactic Ridge Observed with Suzaku
, 2008 In order to elucidate origin of the Galactic Ridge X-ray Emission, we
analyzed Suzaku data taken at various regions along the Galactic plane and
studied their Fe-K emission line features.Ebisawa, Ken, Ezoe, Yuichiro, Koyama, Katsuji, Matsumoto, Hironori, Takahashi, Hiromitsu, Tanaka, Yasuo, Yamasaki, Noriko Y., Yamauchi, Shigeo +7 morecore +1 more sourceTowards the second H.E.S.S. galactic plane catalogue
Proceedings of 38th International Cosmic Ray Conference — PoS(ICRC2023), 2023 The H.E.S.S. Galactic Plane Survey (HGPS), carried out between 2004 and 2013, is the most extensive survey of our Galaxy at very-high energies that covers the southern sky. Since the first HPGS catalogue release, the new observations accumulated provide a deeper scan of many Galactic sources, and a number of improvements have been made at various ...Remy, Q. ; https://orcid.org/0000-0002-8815-6530, Aharonian, F. ; https://orcid.org/0000-0003-1157-3915, Ait-Benkhali, F., Alkan, A., Aschersleben, J., Ashkar, H., Backes, M., Baktash, A., Barbosa Martins, V., Barnacka, A., Barnard, J., Batzofin, R., Becherini, Y., Beck, G., Berge, D., Bernloehr, K. ; https://orcid.org/0000-0001-8065-3252, Bi, B., Boettcher, M., Boisson, C., Bolmont, J., de Bony, M., Borowska, J., Bouyahiaoui, M. ; https://orcid.org/0000-0002-3982-175X, Bradascio, F., Breuhaus, M. ; https://orcid.org/0000-0003-0268-5122, Brose, R., Brown, A., Brun, F., Bruno, B., Bulik, T., Burger-Scheidlin, C., Bylund, T., Cangemi, F., Caroff, S., Casanova, S., Cecil, R., Celic, J., Cerruti, M., Chambéry, P., Chand, T., Chandra, S., Chen, A., Chibueze, J., Chibueze, O., Collins, T., Cotter, G., Cristofari, P., Damascene Mbarubucyeye, J., Davids, I., Davies, J., de Jonge, L., Devin, J., Djannati-Ataï, A., Djuvsland, J. ; https://orcid.org/0000-0002-6488-8219, Dmytriiev, A., Doroshenko, V., Dreyer, L., Du Plessis, L., Egberts, K., Einecke, S., Ernenwein, J., Fegan, S., Feijen, K., Fichet de Clairfontaine, G., Fontaine, G., Frans, L., Fuessling, M., Funk, S., Gabici, S., Gallant, Y., Ghafourizadeh, S., Giavitto, G., Giunti, L., Glawion, D., Glicenstein, J., Glombitza, J., Goswami, P., Grolleron, G., Grondin, M., Haerer, L. ; https://orcid.org/0000-0002-5377-0493, Hattingh, S., Haupt, M., Hermann, G. ; https://orcid.org/0000-0002-4595-1032, Hinton, J. ; https://orcid.org/0000-0002-1031-7760, Hofmann, W. ; https://orcid.org/0000-0001-8295-0648, Holch, T., Holler, M., Horns, D., Huang, Z., Jaitly, A., Jamrozy, M., Jankowsky, F., Jardin-Blicq, A., Joshi, V., Jung-Richardt, I., Kasai, E., Katarzynski, K., Katjaita, H., Khangulyan, D., Khatoon, R., Khelifi, B., Klepser, S., Kluzniak, W., Komin, N., Konno, R., Kosack, K., Kostunin, D., Kundu, A., Lamanna, G., Lang, R., Le Stum, S., Lefranc, V., Leitl, F., Lemiere, A., Lemoine-Goumard, M., Lenain, J., Leuschner, F., Luashvili, A., Lypova, I., Mackey, J., Malyshev, D., Malyshev, D., Marandon, V., Marcowith, A., Marinos, P., Marti'i-Devesa, G., Marx, R., Maurin, G., Mehta, A., Meintjes, P., Meyer, M., Mitchell, A., Moderski, R., Mohrmann, L. ; https://orcid.org/0000-0002-9667-8654, Montanari, A., Moore, C., Moulin, E., Murach, T., Nakashima, K., de Naurois, M., Ndiyavala, H., Niemiec, J., Noel, A., O'Brien, P., Ohm, S., Olivera Nieto, L. ; https://orcid.org/0000-0002-9105-0518, de Ona-Wilhelmi, E., Ostrowski, M., Oukacha, E., Panny, S., Panter, M., Parsons, D., Pensec, U., Peron, G., Pita, S., Poireau, V., Prokhorov, D., Prokoph, H., Puehlhofer, G., Punch, M., Quirrenbach, A., Regeard, M., Reichherzer, P., Reimer, A., Reimer, O., Reis, I., Ren, H. ; https://orcid.org/0000-0003-0221-2560, Renaud, M., Reville, B. ; https://orcid.org/0000-0002-3778-1432, Rieger, F. ; https://orcid.org/0000-0003-1334-2993, Roellinghoff, G., Rol, E., Rowell, G., Rudak, B., Rueda Ricarte, H., Ruiz Velasco, E. ; https://orcid.org/0000-0001-6939-7825, Sabri, K., Sahakian, V., Sailer, S. ; https://orcid.org/0000-0001-8273-8495, Salzmann, H., Sanchez, D., Santangelo, A., Sasaki, M., Schaefer, J., Schuessler, F., Schutte, H., Senniappan, M., Shapopi, J., Shilunga, S., Shiningayamwe, K., Sol, H., Spackman, H., Specovius, A., Spencer, S., Stawarz, L., Steenkamp, R., Stegmann, C., Steinmassl, S. ; https://orcid.org/0000-0002-2865-8563, Steppa, C., Streil, K., Veh, J. +200 moreopenaire +4 more sourcesSearch for variable gamma-ray emission from the Galactic plane in the
Fermi data
, 2012 High-energy gamma-ray emission from the Galactic plane above ~100 MeV is
composed of three main contributions: diffuse emission from cosmic ray
interactions in the interstellar medium, emission from extended sources, such
as supernova remnants and pulsar A. Lutovinov, A. Neronov, Abdo, Abdo, Abdo, Abdo, Abdo, Abdo, Ackermann, Aharonian, Aharonian, Albert, Albert, Atwood, D. Malyshev, Fichtel, Frail, Hunter, M. Chernyakova, Nolan, Telezhinsky +20 morecore +1 more source
