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Vela C
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Title: HOBYS' view of Vela C and W48: a ridge and a mini-starburst Authors: T. Hill, Q. Nguyen Luong, F. Motte, P. Didelon, V. Minier, the HOBYS consortium We present recent results from the Herschel HOBYS guaranteed time key program of the Vela C and W48 star-forming complexes. We examine the column...
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Evaporating gaseous globules
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Title: Photoevaporating Proplyd-like objects in Cygnus OB2 Authors: Nicholas J. Wright, Jeremy J. Drake, Janet E. Drew, Mario G. Guarcello, Robert A. Gutermuth, Joseph L. Hora, Kathleen E. Kraemer We report the discovery of ten proplyd-like objects in the vicinity of the massive OB associati...
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G308.3-1.4
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Title: X-ray properties of G308.3-1.4 and its central compact object Authors: K. A. Seo (1), C. Y. Hui (1), R. H. H. Huang (2), L. Trepl (3), T.-N. Lu (2), A. K. H. Kong (2), F. M. Walter (4) ((1) Chungnam National University, (2) National Tsing Hua University, (3) Universitaet Jena, (4) Stony Brook Uni...
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HR7355
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Title: The most rapidly rotating He-strong emission line star: HR7355 Authors: Th. Rivinius (1), S. Stefl (1), R.H.D. Townsend (2), D. Baade (3) ((1) ESO - Chile, (2) Bartol Research Institute, University of Delaware, (3) ESO - Garching) Using archival spectroscopic and photometric data, we sea...
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Canis Major Dwarf Galaxy
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The Canis Major Dwarf Galaxy was first discovered in November 2003 by an international team of French, Italian, British and Australian astronomers. Although closer to the Earth than the centre of the galaxy itself, the Canis Major Dwarf Galaxy was difficult to detect as it is located behind the pla...
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NGC 4372
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Title: On the impossible NGC 4372 V1 and V2: an extended AGB to the [Fe/H] = -2.2 cluster Authors: Iain McDonald, Albert A. Zijlstra, Andry Rajoelimanana, Christian I. Johnson The asymptotic giant branch (AGB) of the globular cluster NGC 4372 appears to extend to unexpectedly high luminosities. W...
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Interstellar medium
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Title: Implications of the SPEAR FUV Maps on Our Understanding of the ISM Authors: Eric J. Korpela (1), Martin Sirk (1), Jerry Edelstein (1), Kwangil Seon (2), Kyoung-Wook Min (3), Wonyong Han (2) ((1) Space Sciences Laboratory, University of California (2) Korea Astronomy and Space Science Inst...
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Swift J045106.8 -694803
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Possible new Be/X-ray (HMXB) binary system, with a 187 s X-ray period and 21.6 day optical period, in the Large Magellanic Cloud. Position(2000): RA = 04:51:06.8, Dec -69:48:03.2 Uncertainty 3.5 arcseconds
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Abell 35
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Title: BD-22 3467, a DAO-type star exciting the nebula Abell 35 Authors: M. Ziegler (1), T. Rauch (1), K. Werner (1), J. Koeppen (2), J. W. Kruk (3) ((1) Institute for Astronomy and Astrophysics, Kepler Center for Astro and Particle Physics, Eberhard Karls University, Tuebingen, Germany, (2) Obse...
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Gliese 229
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Gliese 229 (also written as Gl 229 or GJ 229) is a red dwarf star about 19 light years away in the constellation Lepus. It has 58% of the mass of the Sun, 69% of the Sun's radius, and a very low projected rotation velocity of 1 km/s at the stellar equator. [url=http://en.wikipedia.org/wiki/Gliese_229B...
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HESS J1303-631
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Title: Identification of HESS J1303-631 as a Pulsar Wind Nebula through gamma-ray, X-ray and radio observations Authors: The H.E.S.S. Collaboration: A. Abramowski, F. Acero, F. Aharonian, A.G. Akhperjanian, G. Anton, S. Balenderan, A. Balzer, A. Barnacka, Y. Becherini, J. Becker, K. Bernlöh...
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RCW173
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Title: An obscured cluster associated with the HII region RCW173 Authors: Amparo Marco, Ignacio Negueruela (University of Alicante, Spain) The discovery of several clusters of red supergiants towards l=24-30 deg has triggered interest in this area of the Galactic plane, where lines of sight ar...
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Stellar bow shocks
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Title: Energetics of nearby stellar bow shocks Authors: Paula Benaglia The latest survey of stellar bow shocks (Peri et al. 2012) lists 28 candidates detected at IR wavelengths, associated with massive, early-type stars up to 3 kpc, along with the geometrical parameters of the structures found....
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Gamma-Ray Binaries
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Title: Revealing Gamma-Ray Binaries Authors: I. F. Mirabel Recent ground based and space telescopes that detect high energy photons from a few up to hundreds of gigaelectron volts (GeV) have opened a new window on the universe. However, because of the relatively poor angular resolution of these t...
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Z Andromedae
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The symbiotic variable star Z Andromedae is in outburst. The star is currently at magnitude 9.0 The cataclysmic variable star is a prototype for symbiotic variables (ZANDs). The system consists of a primary white dwarf and a secondary M giant star. Apparent magnitude: (V) 10.53 Max magnitude...
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