Results 11 to 20 of about 418,206 (216)
The Full-fledged Dwarf Irregular Galaxy Leo A [PDF]
The Astrophysical Journal, 2004 International audienceWe have studied Leo A, an isolated and extremely gas-rich dwarf irregular galaxy of very low stellar mass and metallicity. Ages of the stellar populations in Leo A range from ~10 Myr to ~10 Gyr.Vladas Vansevičius, Donatas Narbutis, Nobuo Arimoto, Naoyuki Tamura, Ohta, Kouji, Tamura, Naoyuki, Jablonka, Pascale, Narbutis, Donatas, Chisato Ikuta, Vansevicius, Vladas, Pascale Jablonka, Yoshihiko Yamada, Stonkute, Rima, Valdas Vansevičius, Kouji Ohta, Takashi Hasegawa, Rima Stonkutė, Yamada, Yoshihiko, Hasegawa, Takashi, Arimoto, Nobuo, Ikuta, Chisato +20 morecore +4 more sourcesA Young Star Cluster in the Leo a Galaxy
Open Astronomy, 2015 We report a serendipitous discovery of a star cluster in the dwarf irregular galaxy Leo A. Young age (~28 Myr) and low mass (~510 M⊙) estimates are based on the isochrone fit assuming a metallicity derived for HII regions (Z = 0.0007).Stonkutė R., Narbutis D., Bridžius A., Leščinskaitė A., Vansevičius V. +4 moredoaj +2 more sourcesSearch for dark matter annihilation in the Wolf-Lundmark-Melotte dwarf irregular galaxy with HESS [PDF]
, 2021 We search for an indirect signal of dark matter through very high-energy γ rays from the Wolf-Lundmark-Melotte (WLM) dwarf irregular galaxy. The pair annihilation of dark matter particles would produce Standard Model particles in the final state such as ...A Reimer (7601036), C van Rensburg (7722008), Y Uchiyama (7721999), A Dmytriiev (7721588), P Marchegiani (7789214), H Ndiyavala (7721810), M Panter (7721834), V Poireau (7721852), G Vasileiadis (7722014), J Mackey (7806869), A Barnacka (9044552), M Buechele (7728818), A Nayerhoda (7770320), M Bryan (7721522), U Katz (7720766), M Tluczykont (7601051), M Spir-Jacob (7721957), R Terrier (7721981), M Sasaki (4487422), H Sol (7721951), L Tomankova (9044579), S Casanova (7721543), D Khangulyan (7721708), B Khelifi (7721711), V Joshi (7770257), P Brun (7721519), H Ashkar (7806848), C Deil (7721573), D Tiziani (7721984), S Raab (7721873), C Steppa (7721969), E de Ona Wilhelmi (8458176), M Holler (7721672), A Quirrenbach (7721870), J Dyks (7721600), F Rieger (7721882), R Rauth (7721876), S Fegan (7721615), S Sailer (8458182), T Lohse (7721753), JF Glicenstein (7721642), HJ Volk (7753970), E Moulin (7721801), R White (7722047), C Boisson (7721501), M Lemoine-Goumard (7721744), G Maurin (7721783), O Reimer (7601039), C Armand (7721477), DJ van der Walt (7722002), L Stawarz (7721960), M Horbe (11418179), R Steenkamp (7721963), D Gottschall (7721645), A Lemiere (7721741), D Glawion (7721639), D Malyshev (7721765), TL Holch (7721669), J Damascene Mbarubucyeye (9913347), S Chandra (7721555), Nu Komin (8458173), M Jamrozy (7721684), R Konno (9044564), S Ohm (7721825), P Reichherzer (10653149), J Hahn (7721651), B van Soelen (7722011), V Barbosa Martins (8458167), A Carosi (7721540), J Veh (7722017), M de Bony de Lavergne (10653113), F Eichhorn (9044555), HM Schutte (8458185), JA Hinton (7721663), L Giunti (8458170), M Tsirou (7721990), M Breuhaus (7806854), M-H Grondin (7721648), G Giavitto (7721636), V Sahakian (7721897), R Zanin (7722062), C Arcaro (7721474), A Mares (7806875), V Doroshenko (7721594), M Fuessling (7721624), I Jung-Richardt (7721696), G Peron (10653143), F Aharonian (7677791), L Rinchiuso (7721885), G Fichet de Clairfontaine (10653122), P DeWilt (7806860), DA Prokhorov (7721858), H Prokoph (7721861), T Bylund (7721531), YA Gallant (7721630), S Klepser (7721717), J Bolmont (7721504), F Niederwanger (7721813), J Niemiec (7721816), G Rowell (7677830), Q Remy (7806881), R Adam (7806845), V Baghmanyan (9044549), F Ait Benkhali (8458164), S Panny (10653140), A Priyana Noel (8458179), C Venter (7722020), C Hoischen (7721666), A Santangelo (7721906), H Odaka (7721822), E Ruiz-Velasco (7721894), PJ Meintjes (7721786), AS Seyffert (7721933), Q Piel (7721849), M Haupt (7721654), A Sinha (7721948), J-P Ernenwein (7721609), R Marx (7721780), M Mohamed (7721795), C Duffy (7736573), K Nakashima (9044570), F Brun (7721516), G Lamanna (7721732), Z Wadiasingh (7722038), AM Taylor (7721978), AA Zdziarski (7722065), R Tuffs (7721996), M Scalici (9044573), D Zargaryan (9044582), S Caroff (7721537), F Jankowsky (7721690), G Puhlhofer (7601030), A Donath (7721591), S Schwemmer (7721924), A Yusafzai (10653167), J Zorn (7722074), S Funk (691019), M Meyer (557509), T Vuillaume (7722035), K Katarzynski (7721702), W Hofmann (7717322), M Curylo (7806857), M de Naurois (7721807), K Shiningayamwe (7721942), S Steinmassl (10653158), R Simoni (7721945), M Kreter (7753649), I Lypova (7721762), M Seglar-Arroyo (7721927), C Romoli (7721888), R Moderski (7721792), M Bottcher (7721498), C Levy (7806866), RD Parsons (7721837), Y Becherini (7721483), T Takahashi (841902), A Montanari (10653134), J Majumdar (7806872), P Vincent (7722023), J Vink (7722026), C Moore (7713326), S Spencer (9044576), ID Davids (7721570), MA Kastendieck (7721699), C Stegmann (7721966), J-P Lenain (7721747), A Specovius (7721954), M Backes (7707428), M Barnard (7338422), B Peyaud (7721846), J Devin (7721576), D Kostunin (7793858), A Wierzcholska (7722050), C van Eldik (7722005), S Zouari (10653170), DA Sanchez (7721903), T Armstrong (9044546), S Gabici (7721627), B Bi (9913338), D Horns (7677809), H Abdallah (7784381), EO Anguner (7721468), M Senniappan (7721930), L Olivera-Nieto (10653137), D Jankowsky (7721687), A Jardin-Blicq (7770254), SJ Wagner (7722041), A Chen (7721561), G Cotter (7729403), V Marandon (7721768), M Zacharias (7722059), M Ostrowski (7721828), F Werner (7770389), S Zhu (7730540), M Punch (7721867), L Mohrmann (7721798), B Rudak (7721891), Yu Wun Wong (10653164), G Fontaine (7721621), T Chand (7721552), S Pita (7601027), G Marti-Devesa (7721777), K Bernloehr (7721492), J Muller (7806878), M Renaud (7721879), T Bulik (7721528), J Davies (7777496), L Dirson (7721582), A Zech (7722068), N Zywucka (7722077), K Feijen (7793855), A Fiasson (7721618), J Watson (7788164), L Oakes (7721819), K Kosack (7721726), G Hermann (7601015), W Kluzniak (7721720), T Tavernier (7721975), E Kasai (9913359), P O'Brien (7678940), S Einecke (7736576), D Berge (7721489), P Morris (9044567), U Schwanke (7721921), K Egberts (7721603), T Murach (7721804), F Schussler (7721912), C Trichard (7721987), A Marcowith (7721771), A Djannati-Atai (7721585), L Sun (7715189), G Emery (7721606), N Shafi (7721936), D Huber (7721675) +233 morecore +8 more sourcesBacterial Lysis Observation Over Time Assay (BLOTS) for High-Throughput Isolation, Sequencing, and Characterization of Bacteriophages. [PDF]
Curr ProtocAbstract
Phages remain severely under‐sampled, largely due to the limitations of current isolation methods, which are labor‐intensive, low‐throughput, and often restricted to a narrow set of bacterial hosts. To address this gap, we developed a robust and scalable field‐to‐genome workflow that leverages laboratory automation to screen environmental ...Pang SJL, Wee SK, Lee BGW, Yap O, Yap EPH. +4 moreeuropepmc +2 more sourcesTHE OUTER DISKS OF DWARF IRREGULAR GALAXIES [PDF]
The Astronomical Journal, 2011 AJ, in ...Hunter, Deidre A., Elmegreen, Bruce G., Oh, Se-Heon, Anderson, Ed, Nordgren, Tyler E., Massey, Philip, Wilsey, Nick, Riabokin, Malanka +7 moreopenaire +2 more sourcesMagnetic Fields in Irregular Galaxies [PDF]
Proceedings of the International Astronomical Union, 2008 Magnetic fields are an important component of the interstellar medium, especially in low-mass galaxies like irregulars where the magnetic pressure may be significant. However, few irregular galaxies have observed magnetic field structures. Using the VLA, the GBT, and the ATCA, we have observed several irregular galaxies in the radio continuum to ...Kepley, Amanda A., Muehle, Stefanie, Wilcots, Eric M., Everett, John, Zweibel, Ellen, Robishaw, Timothy, Heiles, Carl +6 moreopenaire +4 more sourcesGalaxy masses [PDF]
, 2014 Galaxy masses play a fundamental role in our understanding of structure formation models. This review addresses the variety and reliability of mass estimators that pertain to stars, gas, and dark matter.Courteau, Stephane, Cappellari, Michele, Hoekstra, Henk, Treu, Tommaso, Widrow, Lawrence M., Emsellem, Eric, Maraston, Claudia, Koopmans, L. V. E., Dutton, Aaron A., Mamon, Gary A., de Jong, Roelof S. +10 morecore +1 more sourceLopsidedness in dwarf irregular galaxies [PDF]
Monthly Notices of the Royal Astronomical Society, 2000 We quantify the amplitude of the lopsidedness, the azimuthal angular asymmetry index, and the concentration of star forming regions, as represented by the distribution of the H$α$ emission, in a sample of 78 late-type irregular galaxies. We bin the observed galaxies in two groups representing blue compact galaxies (BCDs) and low surface brightness ...Heller, Ana B., Brosch, Noah, Almoznino, Elchanan, van Zee, Liese, Salzer, John J. +4 moreopenaire +2 more sources
