In the spectrum of an emission-line region ejected from the massive star Eta Carinae, called the strontium filament (SrF), forbidden lines from many elements, in particular [Sr II] and [Ti II], are observed. These lines are strong in this specific region and valuable for plasma diagnostics. Forbidden lines are not easily produced in laboratory light sources and the atomic parameters for these lines can thus not be measured in a straightforward way. We use a combination of laboratory and astrophysical measurements to determine transition probabilities for the [Ti II] lines. Lifetimes for metastable levels in Ti II are measured using a laser probing technique on a stored ion beam at CRYRING, MSL, Stockholm. Branching fractions from some of th...
During a series of HST/STIS observations of Eta Carinae and associatedejecta, we noticed a peculiar ...
We have discovered four extremely surprising emission lines of strontiumin ejecta near eta Carinae. ...
We report lifetime measurements of the 6 levels in the 3d(6)(5D)4d e(6)G term in Fe II at an energy ...
Context. In many plasmas, long-lived metastable atomic levels are depopulated by collisions (quenche...
Eta Carinae is one of the most massive and luminous stars in the Galaxy. A huge bipolar nebula and a...
Context. Accurate transition probabilities for forbidden lines are important diagnostic parameters f...
We report on experimental transition probabilities for thirteenforbidden [Fe II] lines originating f...
We report on experimental transition probabilities for thirteen forbidden [Fe II] lines originating ...
We report on experimental transition probabilities for thirteen forbidden [Fe II] lines originating ...
peer reviewedThis paper presents new theoretical lifetimes of metastable levels in singly ionized ti...
peer reviewedThis paper presents new theoretical lifetimes of metastable levels in singly ionized ti...
Parity forbidden radiative transitions from metastable levels are observed in spectra of low-density...
Parity forbidden radiative transitions from metastable levels are observed in spectra of low-density...
In dilute astrophysical plasmas, such as planetary nebulae and H ii regions, strong lines appear tha...
We report measurements of the relative intensities of 81 emission linesof Fe II between 160 nm and 3...
During a series of HST/STIS observations of Eta Carinae and associatedejecta, we noticed a peculiar ...
We have discovered four extremely surprising emission lines of strontiumin ejecta near eta Carinae. ...
We report lifetime measurements of the 6 levels in the 3d(6)(5D)4d e(6)G term in Fe II at an energy ...
Context. In many plasmas, long-lived metastable atomic levels are depopulated by collisions (quenche...
Eta Carinae is one of the most massive and luminous stars in the Galaxy. A huge bipolar nebula and a...
Context. Accurate transition probabilities for forbidden lines are important diagnostic parameters f...
We report on experimental transition probabilities for thirteenforbidden [Fe II] lines originating f...
We report on experimental transition probabilities for thirteen forbidden [Fe II] lines originating ...
We report on experimental transition probabilities for thirteen forbidden [Fe II] lines originating ...
peer reviewedThis paper presents new theoretical lifetimes of metastable levels in singly ionized ti...
peer reviewedThis paper presents new theoretical lifetimes of metastable levels in singly ionized ti...
Parity forbidden radiative transitions from metastable levels are observed in spectra of low-density...
Parity forbidden radiative transitions from metastable levels are observed in spectra of low-density...
In dilute astrophysical plasmas, such as planetary nebulae and H ii regions, strong lines appear tha...
We report measurements of the relative intensities of 81 emission linesof Fe II between 160 nm and 3...
During a series of HST/STIS observations of Eta Carinae and associatedejecta, we noticed a peculiar ...
We have discovered four extremely surprising emission lines of strontiumin ejecta near eta Carinae. ...
We report lifetime measurements of the 6 levels in the 3d(6)(5D)4d e(6)G term in Fe II at an energy ...