IGR J17091-3624 (English Wikipedia)

Analysis of information sources in references of the Wikipedia article "IGR J17091-3624" in English language version.

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Xu, Y.; García, J.A.; Fürst, F.; Harrison, F.A.; Walton, D.J.; Tomsick, J.A.; Bachetti, M.; King, A.L.; Madsen, K.K.; Miller, J.M.; Grinberg, V. (2017). "Spectral and Timing Properties of IGR J17091–3624 in the Rising Hard State During Its 2016 Outburst". The Astrophysical Journal. 851 (2): 103. arXiv:1711.04421. Bibcode:2017ApJ...851..103X. doi:10.3847/1538-4357/aa9ab4. S2CID 119414510.
Rao, Anjali; Vadawale, S. V. (12 September 2012). "Why is IGR J17091–3624 so faint?". The Astrophysical Journal. 757 (1): 1. arXiv:1209.2506. Bibcode:2012ApJ...757L..12R. doi:10.1088/2041-8205/757/1/L12. S2CID 118636206.
Rao, Anjali; Vadawale, S. V. (12 September 2012). "Why is IGR J17091–3624 so faint?". The Astrophysical Journal. 757 (1): 2. arXiv:1209.2506. Bibcode:2012ApJ...757L..12R. doi:10.1088/2041-8205/757/1/L12. S2CID 118636206.

Erik Kuulkers (April 19, 2003). "IGR J17091-3624". astronomerstelegram.org. Retrieved January 17, 2013.

Xu, Y.; García, J.A.; Fürst, F.; Harrison, F.A.; Walton, D.J.; Tomsick, J.A.; Bachetti, M.; King, A.L.; Madsen, K.K.; Miller, J.M.; Grinberg, V. (2017). "Spectral and Timing Properties of IGR J17091–3624 in the Rising Hard State During Its 2016 Outburst". The Astrophysical Journal. 851 (2): 103. arXiv:1711.04421. Bibcode:2017ApJ...851..103X. doi:10.3847/1538-4357/aa9ab4. S2CID 119414510.
Rao, Anjali; Vadawale, S. V. (12 September 2012). "Why is IGR J17091–3624 so faint?". The Astrophysical Journal. 757 (1): 1. arXiv:1209.2506. Bibcode:2012ApJ...757L..12R. doi:10.1088/2041-8205/757/1/L12. S2CID 118636206.
Rao, Anjali; Vadawale, S. V. (12 September 2012). "Why is IGR J17091–3624 so faint?". The Astrophysical Journal. 757 (1): 2. arXiv:1209.2506. Bibcode:2012ApJ...757L..12R. doi:10.1088/2041-8205/757/1/L12. S2CID 118636206.

Ashley King; et al. (February 21, 2012). "IGR J17091: Chandra Finds Fastest Winds". NASA/Harvard. Retrieved September 27, 2012.
Ashley King; et al. (February 21, 2012). "Chandra Finds Fastest Winds from Stellar Black Hole". NASA. Retrieved September 27, 2012.
Ashley King; et al. (February 21, 2012). "Chandra Finds Fastest Winds from Stellar Black Hole". NASA. Retrieved September 27, 2012.

Xu, Y.; García, J.A.; Fürst, F.; Harrison, F.A.; Walton, D.J.; Tomsick, J.A.; Bachetti, M.; King, A.L.; Madsen, K.K.; Miller, J.M.; Grinberg, V. (2017). "Spectral and Timing Properties of IGR J17091–3624 in the Rising Hard State During Its 2016 Outburst". The Astrophysical Journal. 851 (2): 103. arXiv:1711.04421. Bibcode:2017ApJ...851..103X. doi:10.3847/1538-4357/aa9ab4. S2CID 119414510.
Rao, Anjali; Vadawale, S. V. (12 September 2012). "Why is IGR J17091–3624 so faint?". The Astrophysical Journal. 757 (1): 1. arXiv:1209.2506. Bibcode:2012ApJ...757L..12R. doi:10.1088/2041-8205/757/1/L12. S2CID 118636206.
Rao, Anjali; Vadawale, S. V. (12 September 2012). "Why is IGR J17091–3624 so faint?". The Astrophysical Journal. 757 (1): 2. arXiv:1209.2506. Bibcode:2012ApJ...757L..12R. doi:10.1088/2041-8205/757/1/L12. S2CID 118636206.

Xu, Y.; García, J.A.; Fürst, F.; Harrison, F.A.; Walton, D.J.; Tomsick, J.A.; Bachetti, M.; King, A.L.; Madsen, K.K.; Miller, J.M.; Grinberg, V. (2017). "Spectral and Timing Properties of IGR J17091–3624 in the Rising Hard State During Its 2016 Outburst". The Astrophysical Journal. 851 (2): 103. arXiv:1711.04421. Bibcode:2017ApJ...851..103X. doi:10.3847/1538-4357/aa9ab4. S2CID 119414510.
Rao, Anjali; Vadawale, S. V. (12 September 2012). "Why is IGR J17091–3624 so faint?". The Astrophysical Journal. 757 (1): 1. arXiv:1209.2506. Bibcode:2012ApJ...757L..12R. doi:10.1088/2041-8205/757/1/L12. S2CID 118636206.
Rao, Anjali; Vadawale, S. V. (12 September 2012). "Why is IGR J17091–3624 so faint?". The Astrophysical Journal. 757 (1): 2. arXiv:1209.2506. Bibcode:2012ApJ...757L..12R. doi:10.1088/2041-8205/757/1/L12. S2CID 118636206.

Charles Q. Choi (August 24, 2012). "Strangest Black Holes in the Universe, pg 9". Space.com. Retrieved September 27, 2012.