Search

24 Feb 2012: In prep. ABSTRACT. We present new MIDI interferometric and VISIR spectroscopic observations ofHD113766 and HD172555.

8 Jul 2008: For a parent with an orbit defined by a ande broken up at a true anomaly f , the new orbital elements are.

23 Mar 2007: 2005)(e.g., Fig. 1), the main new result of Su et al. ... used the new distributions of 24 and 70 µm excesses asa function of age shown in Fig.

7 Jul 2012: 2009; Bryden et al. 2009;Dodson-Robinson et al. 2011). However, there is new tentative ev-idence that nearby stars with low-mass planetary systems are morelikely to harbour debris than

5 Jul 2011: Wealso present new SPIRE images of the disc at 250 µm, as well as new constraints on the discfrom SCUBA-2, mid-IR and scattered light imaging. ... Stock et al. (2010) present new 10 µm nulling interferometrydata from the Keck Interferometer Nuller (KIN)

5 Oct 2007: Spitzer. IRS observations of the Deep Impact experiment in July 2005 created a new paradigm for under-. ... new species was allowed, and only species that reduced the χ2ν below the 95% confidence limit.

29 Apr 2008: In3 the various observational and analysistechniques employed for each instrument are outlined, and insection4 a new method of placing quantifiable extension lim-its on unresolved disk images is described. ... 4.1. A new method of determining extension

25 Nov 2010: arX. iv:1. 011. 4858. v1 [. astr. o-ph. EP]. 22. Nov. 201. 0Mon. Not. R. Astron. Soc. 000, 000–000 (0000) Printed 23 November 2010 (MN LATEX style file v2.2). Collisional Evolution of Irregular Satellite Swarms:. Detectable Dust around Solar

16 Nov 2021: a new solution for a star of a different totalmass M ′ simply by multiplying the other physical variables by appropriatescaling factors.

10 Nov 2010: 5. Discussion and conclusions. Using new mid-IR images at 18 and 25µm, we have confirmedthe previously observed brightness asymmetry discovered byTelesco et al. ... 350,Hipparcos, the New Reduction of the Raw Data. Wahhaj, Z., Koerner, D.