Herschel observations show modestly depleted oxygen ( Keane et al. The MAPS observations show the presence of spectacular, large-scale CO spiral arms ( MAPS XIX, Huang et al. 2008) and bright lines associated with photochemistry and small organics ( Öberg et al. The GM Aur disk has been observed in several gas tracers, with indications of non-Keplerian CO emission ( Dutrey et al. 2018) and a small inner disk inside this central gap ( Huang et al. High resolution continuum observations at cm and mm wavelengths showed that the outer disk consists of several nested rings surrounded by diffuse continuum emission to ~270 au ( Macías et al. The large dust cavity (~35 au) was first inferred from SED modeling ( Marsh & Mahoney 1992) and later confirmed by direct imaging using mm observations ( Hughes et al.
GM Aur is a ~3-10 Myr T Tauri star in the Taurus-Auriga star-forming region hosting a transition disk, i.e., a disk large with a large inner gap or cavity. Spitzer observations showed weak OH and H 2O emission in the inner disk, suggesting intermediate water depletion ( Banzatti et al. No depletions were found in nitrogen, resulting in an elevated gas-phase N/O ratio ( Cleeves et al. Modeling indicates that CO is underabundant by a factor of ~20 compared to molecular clouds due to missing gas-phase carbon and oxygen ( Cleeves et al. 2011) and shows a striking double-ring structure in DCO +, due to a change in gas-phase C and O abundance at the pebble disk edge ( Öberg et al. IM Lup has been been observed in several molecular lines ( Öberg et al. The outer portion of the CO gas disk is diffuse and envelope-like, potentially indicating the presence of an external photoevaporative wind ( Haworth et al. 2018).ĭespite its youth, the IM Lup disk shows evidence of grain growth ( Lommen et al. 2018b), while scattered light observations show a highly flared, multi-ringed disk in micron-sized dust grains ( Avenhaus et al. 2016).Ĭontinuum images reveal the presence of spiral arms in mm grains ( Huang et al. 2018a) and a CO disk out to ~900 au ( Cleeves et al. IM Lup has the largest pebble disk (~260 au) in the DSHARP sample ( Huang et al. And the installation was awful.Please a.IM Lup is a young (~1 Myr), Solar-mass star that hosts a massive and radially-extended disk. Some of it is freeish but I don't feel like it worked great.
Salutations, I'm seeking a free vulnerability scanner that doesn't suck too bad.I tried OpenVAS/Greenbone but it seems it has been more or less paywalled. I've used the EICAR test string to test that anti-virus systems work:ĭownload Anti Malware Testfile – Eicar Is there an equivalent for phishing? Or any other suggestions for running a quic. Hi,I need to test an anti-Phishing policy on our email system. Is there a Phishing equivalent to the EICAR test string? Security.But I know we have a lot of members who enjoy space news so you may enjoy this on. Not a lot of information technology news that happened on July 6, unless you want to talk about IBM buying Lotus back in 1995. 6, Broadcom & VMware, CAPSTONE, & more Spiceworks Originals Snap! Cyberattacks in Brazil, WiFi 5 vs.Nearly all of our office phones are DT300 DTL-24D-1 desk phones. We upgraded from an SV8100 roughly a year ago by swapping out the SV8100 cards with SV9100 cards installed into the same chassis.
Hello all,We have an NEC SV9100 phone system.