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Staphylococcus aureus asymptomatically colonizes the nasal cavity of mammals, but it is also a leading cause of life-threatening infections. Most human nasal isolates carry Sa3 phages, which integrate into the bacterial hlb gene encoding a sphingomyelinase. The virulence factor-encoding genes carried by the Sa3-phages are highly human-specific, and most animal strains are Sa3 negative. Thus, both insertion and excision of the prophage could potentially confer a fitness advantage to S. aureus. Here, we analyzed the phage life cycle of two Sa3 phages, Φ13 and ΦN315, in different phage-cured S. aureus strains. Based on phage transfer experiments, strains could be classified into low (8325-4, SH1000, and USA300c) and high (MW2c and Newman-c) transfer strains. High-transfer strains promoted the replication of phages, whereas phage adsorption, integration, excision, or recA transcription was not significantly different between strains. RNASeq analyses of replication-deficient lysogens revealed no strain-specific differences in the CI/Mor regulatory switch. However, lytic genes were significantly upregulated in the high transfer strain MW2c Φ13 compared to strain 8325-4 Φ13. By transcriptional start site prediction, new promoter regions within the lytic modules were identified, which are likely targeted by specific host factors. Such host-phage interaction probably accounts for the strain-specific differences in phage replication and transfer frequency. Thus, the genetic makeup of the host strains may determine the rate of phage mobilization, a feature that might impact the speed at which certain strains can achieve host adaptation.
Fulminic acid, HCNO, was first synthesized in the year 1800 and has since then been used numerous times to develop new chemical theories and concepts. Nowadays, research on HCNO is mainly motivated due to its detection in interstellar space in the year 2009. In this thesis, we investigated the interaction of fulminic acid with VUV- and soft X-ray radiation, i.e., radiation that is also present in the interstellar medium. In our study using VUV radiation, we were able to record the photoelectron spectrum of HCNO with high resolution and we were able to simulate the Renner-Teller distorted ground state of the cation using simulation of wavepacket dynamics. We also elucidated the mechanism of the dissociative photoionisation up to 15.3 eV binding energy. Using soft X-ray radiation enables us to ionise or excite the 1s electrons of HCNO. The created state can decay via an Auger-Meitner process, which produces an Auger electron. We measured the kinetic energy of these auger electron and were able to analyse the observed signals using quantum chemical calculations. We also investigated how the ion fragments after the Auger-Meitner process. We observed a site-selectivity, where the initial ionisation/excitation site influenced the product distribution. We were able to explain this observation with a simple thermodynamic argument. This thesis provides a comprehensive description of the interaction of HCNO with ionising radiation. The obtained data may be valuable for the description of the behaviour of HCNO in interstellar space.