Publication data of Podsiadlowski, Philipp:
Link to Inspire
Created with Highcharts 9.0.1
Citations
Citations
w/o self-citaion
self-citaion
1995
2000
2005
2010
2015
2020
2025
0
2500
5000
7500
10000
12500
Created with Highcharts 9.0.1
Publications
publications per year
Publications
Publications per year
Cumulative publications
1995
2000
2005
2010
2015
2020
2025
0
30
60
90
120
150
0
4
8
12
16
20
Created with Highcharts 9.0.1
h-index
h-index
h-index
h-index w/o self-citaion
1995
2000
2005
2010
2015
2020
2025
0
10
20
30
40
50
60
Created with Highcharts 9.0.1
Citations
Breakdown of Most Cited Papers
rest
The role of mass transfer and common envelope evolution in the formation of merging binary black holes
The role of mass transfer and common envelope evolution in the formation of…
The Galactic population of low- and intermediate - mass x-ray binaries
A new class of high-mass x-ray binaries: implications for core collapse and neutron-star recoil
A new class of high-mass x-ray binaries: implications for core collapse and ne…
Remnant evolution after a carbon-oxygen white dwarf merger
Ultra-stripped Type Ic Supernovae from Close Binary Evolution
The Rates of hypernovae and gamma-ray bursts: Implications for their progenitors
The Rates of hypernovae and gamma-ray bursts: Implications for their proge…
The Massive binary companion star to the progenitor of supernova 1993J
The origin of sdb stars (ii)
On the formation history of Galactic double neutron stars
On the formation and evolution of black hole binaries
On the nature and evolution of the unique binary pulsar J1903+0327
The single degenerate channel for the progenitors of type Ia supernovae
The Origin of subdwarf B stars. 1. The Formation channels
Ultra-stripped supernovae: progenitors and fate
The effects of binary evolution on the dynamics of core collapse and neutron - star kicks
The effects of binary evolution on the dynamics of core collapse and neutron …
Evolutionary binary sequences for low- and intermediate-mass x-ray binaries
Common Envelope Evolution: Where we stand and how we can move forward
A new route towards merging massive black holes
Formation of Double Neutron Star Systems
1995
2000
2005
2010
2015
2020
2025
0
2500
5000
7500
10000
12500
Created with Highcharts 9.0.1
Fraction [%]
Breakdown of Most Cited Papers (Fraction)
The role of mass transfer and common envelope evolution in the formation of merging binary black holes
The role of mass transfer and common envelope evolution in the formation of…
The Galactic population of low- and intermediate - mass x-ray binaries
A new class of high-mass x-ray binaries: implications for core collapse and neutron-star recoil
A new class of high-mass x-ray binaries: implications for core collapse and ne…
Remnant evolution after a carbon-oxygen white dwarf merger
Ultra-stripped Type Ic Supernovae from Close Binary Evolution
The Rates of hypernovae and gamma-ray bursts: Implications for their progenitors
The Rates of hypernovae and gamma-ray bursts: Implications for their proge…
The Massive binary companion star to the progenitor of supernova 1993J
The origin of sdb stars (ii)
On the formation history of Galactic double neutron stars
On the formation and evolution of black hole binaries
On the nature and evolution of the unique binary pulsar J1903+0327
The single degenerate channel for the progenitors of type Ia supernovae
The Origin of subdwarf B stars. 1. The Formation channels
Ultra-stripped supernovae: progenitors and fate
The effects of binary evolution on the dynamics of core collapse and neutron - star kicks
The effects of binary evolution on the dynamics of core collapse and neutron …
Evolutionary binary sequences for low- and intermediate-mass x-ray binaries
Common Envelope Evolution: Where we stand and how we can move forward
A new route towards merging massive black holes
Formation of Double Neutron Star Systems
1995
2000
2005
2010
2015
2020
2025
0
25
50
75
100
Created with Highcharts 9.0.1
Citations/1 Year
Citations/Period
Citations / 1 Year
Moving average
1995
2000
2005
2010
2015
2020
2025
0
250
500
750
1000
1250
1 Month
3 Months
6 Months
12 Months